The galaxy exhibits a generally smooth morphology, appearing elliptical in shape, though it is close to round. A bright central bulge dominates the structure, with a gradual decrease in luminosity extending outwards. The color gradient suggests a relatively homogenous stellar population, with a yellowish hue characteristic of older stars. There are no readily apparent spiral arms, dust lanes, or active star-forming regions. There is little to no significant tidal disturbance or signs of recent merging activity.
