The galaxy presents as a generally smooth, elliptical-like structure with a concentrated central bulge. Its color is a yellowish-white hue, suggesting a population of older stars. There is a subtle color gradient, with the central region appearing more yellow and the outer regions trending towards a slightly bluer tint. The overall morphology indicates a lack of significant star formation in the recent past, consistent with a more evolved system. No distinct spiral arms or prominent dust lanes are discernible. The galaxy appears relatively isolated, without obvious signs of tidal interaction or ongoing mergers. A small degree of asymmetry may be present, but it is not pronounced.
