The galaxy exhibits a generally elliptical morphology. A bright, concentrated central bulge dominates the luminosity profile. Extending from the bulge is a faint, diffuse halo. This halo appears asymmetrical, with a noticeable extension or plume of lower surface brightness material projecting away from the main body of the galaxy, possibly indicative of tidal interactions or past merger events. The color gradient suggests a relatively old stellar population, though there may be some bluer regions. The galaxy has a smooth appearance, with minimal indication of spiral arms. There are no obvious dust lanes visible in this image.
