The galaxy presents as a relatively smooth, lenticular-like structure, elongated in shape. A slight bulge is inferred from a central brightening. The color distribution appears non-uniform with a yellowish central region, suggestive of an older stellar population, grading into a bluish outer region that indicates more recent star formation. There is a subtle asymmetry in the color distribution, suggestive of either tidal interactions or internal processes affecting star formation rates. Overall, the galaxy appears quiescent.
