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Our understanding of the lunar farside from orbital remote sensing is limited by the lack of ground-truth constraints from returned samples. China's Chang'e-6 (CE-6) mission plans to land at the southern rim of the Apollo basin in the South Pole-Aitken basin on the lunar farside and return ∼2 kg samples. In this study, we conduct analyses on the local geological context of the CE-6 candidate landing regions, with a focus on the non-mare ejecta. The CE-6 candidate landing region has been divided into three subunits. According to our analyses, the northeastern subunit is adjacent to the lowest elevation (and one of the highest excavation depth) of this region where the materials from the deepest crust may exist. The northwestern subunit is affected by the magnesian ejecta from young crater. Returning these non-mare ejecta will provide key insights into the magnesian lithologies that occurred in the lunar farside, whose petrogenesis is long debated. As for the southern light plains unit, a topographic positive feature (unofficially termed as Mons White) located at the west of the light plains is identified in this work. Three scenarios were proposed for its origin: (1) A volcanic complex built on special magmatism in the SPA basin; (2) Remnants of the central uplift of an ancient impact basin; (3) Target surface folded and uplifted by the Apollo basin impact event. Gradual lithological variations in the Mons White are discovered. The White crater has likely ejected materials with these gradual lithologies into the CE-6 candidate landing regions. The Orientale basin ejecta also exists on the light plains. These non-mare materials, if could be sampled by the CE-6 mission, will significantly help refine the lunar chronostratigraphic system from the pre-Nectarian/Aitkenian to the late Imbrian. Thus, we suggest that landing on the southern light plains will achieve the maximum scientific outcomes for the CE-6 mission, from a perspective of sample diversity. • We conduct analyses on the local geological context of the CE-6 candidate landing regions. • The northeastern subregion is adjacent to the Chawla crater where deep-seated materials may exist. • The northwestern subunit is affected by the magnesian ejecta from young crater. • A topographic positive feature located at the west of the candidate landing region is identified. • Three scenarios were proposed for the origin of the topographic positive feature. [ABSTRACT FROM AUTHOR]