The galaxy presents as a generally smooth object, with a roughly elliptical morphology. It exhibits a concentrated central bulge, with a gradual decrease in luminosity towards its outer regions. There is a slight hint of a disk-like structure, though not clearly defined. The galaxy exhibits a fairly uniform color profile across its entirety, with a general color indicative of an older stellar population. This galaxy exhibits indications of a minor gravitational disturbance, but it is not currently undergoing a major merger event.
