The galaxy presents as a generally smooth and elliptical structure, with a bright central bulge that gradually fades into the outer regions. Its color profile suggests a population of older stars, contributing to the yellowish-orange hue. There is no discernable spiral arm structure or dust lane visible. The overall shape is slightly elongated. Indications suggest the galaxy is relatively massive with modest star formation. There are no obvious signs of a major ongoing merger, though subtle disturbances may be present.
