The galaxy presents as a roughly elliptical, somewhat diffuse object. The central region exhibits a concentrated, bright core, suggestive of a substantial stellar population and potentially an active galactic nucleus. A faint, flattened disk-like structure extends outward from the central bulge. There is a slight bluing on one side of the disk region, indicating the presence of some on going star formation, though overall the galaxy appears relatively smooth and evolved. Some slight asymmetries in the outer regions suggest potential past or ongoing minor gravitational interactions, but the galaxy appears mostly undisturbed.
