The galaxy presents as a fairly smooth, centrally concentrated object. The core exhibits a yellowish hue, which may indicate an older stellar population. The overall shape is moderately elliptical, with some suggestion of a disk-like component. There are subtle hints of spiral structure present, particularly in the outer regions, which appear slightly bluer in color. Some minor disturbances may be present, such as a slight asymmetry, but the galaxy is generally undisturbed. Overall, the galaxy appears to be a relatively massive system with moderate star formation activity.
