The galaxy appears to be an elliptical galaxy. It exhibits a generally smooth morphology, with a concentrated, bright central region. The galaxy's shape is predominantly spheroidal, but shows a slight elongation along one axis. There is no clear evidence of spiral arms or significant dust lanes within the galaxy. The color profile suggests a population of older stars, with the central region appearing yellower. The overall color index indicates a relatively low level of ongoing star formation. Faint, diffuse light extends outward from the main body of the galaxy, forming a halo or envelope. No signs of a major merger event are apparent, with the main body of the galaxy being undisturbed. There are some minor disturbances visible.
