This galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a concentrated central bulge with a gradual decrease in luminosity outwards. The galaxy shows a slightly elongated, round shape. There is a faint disk-like component. There does not seem to be any evidence of major merging activity or significant tidal disturbances. The color gradient suggests a population of older stars, with a possible small amount of ongoing star formation. The overall morphology indicates that this is a rather evolved system with a significant stellar mass.
