The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The color profile suggests a dominant population of older stars, leaning towards the redder end of the spectrum. There is minimal evidence of spiral arm structure or significant dust lanes, although the edges are not perfectly defined. Its overall form is roughly circular, appearing largely undisturbed, with a relatively uniform light distribution across its surface. The absence of prominent blue regions indicates a low rate of ongoing star formation. There is perhaps a slight extension on one side that may indicate tidal interactions. Overall, it appears to be a quiescent galaxy, likely residing in a more evolved state.
