The galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a concentrated central bulge and a more diffuse halo. The light profile suggests a lack of significant spiral arm structure. It displays a generally rounded morphology, with no apparent major distortions indicative of ongoing mergers or tidal interactions. The galaxy exhibits a color gradient, with the central regions appearing more yellow-orange, suggestive of an older stellar population, and the outer regions appearing slightly bluer, indicating the presence of some younger stars or ongoing star formation, albeit at a low rate. The overall color suggests a relatively evolved system with a moderately high stellar mass.
