This galaxy appears to be a relatively smooth, elliptical-like structure with a concentrated central bulge. The galaxy exhibits a radial color gradient, with the core appearing more yellow-orange. This is possibly indicative of an older stellar population dominating the central region. Moving outwards from the core, the galaxy's color shifts to slightly redder hues, suggesting the presence of cooler and potentially older stars in the outer regions as well. The overall shape is nearly circular. There is no obvious indication of spiral arm structure. Slight asymmetry in the outer halo may suggest past interactions.
