The galaxy presents as a relatively compact, elliptical or lenticular system. It exhibits a smooth, centrally concentrated light profile with a noticeable bulge component. The galaxy shows a color gradient, appearing more reddish in the central regions, which may indicate an older stellar population. The outer regions are slightly bluer, suggesting a small degree of ongoing star formation. There is no obvious spiral arm structure or significant dust lane features visible. There's no evidence of an active galactic nucleus or extreme starburst activity given the colors. The overall morphology is suggestive of a galaxy that has largely exhausted its gas supply and is undergoing passive evolution. No tidal tails or other signs of major mergers are apparent, but there might be minor disturbances in the outskirts.
