The galaxy appears as a single, relatively smooth object, with a concentrated central bulge. It presents a near face-on orientation relative to our line of sight. The color profile suggests a population of older stars, particularly in the central regions, with a possible slight reddening. There is a faint suggestion of some disk-like structure surrounding the central bulge. Some minor disturbances are seen around the galaxy, which may suggest a possible interaction with other small galaxies. There are slight color variations, with hints of fainter, bluer regions, which could suggest areas of more recent, though somewhat subdued, star formation. The overall morphology appears to be that of a relatively massive galaxy, possibly an early-type spiral galaxy, given the smoothness.
