The galaxy appears to be a relatively smooth, elliptical-type galaxy, with a concentrated central bulge. Its overall shape is close to circular, indicating a low degree of observed ellipticity. There is no readily apparent disk structure or spiral arm morphology visible in this image. The light profile exhibits a smooth gradient, with a peak in intensity at the nucleus and a gradual decrease in luminosity outwards. The color appears predominantly yellowish-white, suggesting a stellar population dominated by older stars and a relatively low rate of ongoing star formation. No signs of recent or major merging events are observable, with no tidal tails or distorted morphology present. Faint color variations indicate that some regions may have slightly different stellar populations or dust content, but overall the galaxy has a homogenous appearance.
