The galaxy presents a largely smooth and elliptical morphology. It exhibits a concentrated central bulge that appears predominantly yellow, indicating a population of older stars. The outer regions show a gradual decline in brightness, with a subtle transition to a slightly bluer hue. There is a slight indication of a disk-like structure. There is no indication of major disturbances or ongoing mergers, though there could be a minor disturbance present. Overall, the galaxy presents a mostly smooth, round appearance.
