The galaxy presents as a relatively compact, elliptical-like system. Its morphology appears largely smooth, with minimal evidence of spiral arms or distinct features. The light distribution is centrally concentrated, with a gradual decrease in surface brightness outwards. The galaxy appears to be relatively round in shape, showing minimal ellipticity or distortion. Coloration is dominated by redder hues, indicative of an older stellar population and a likely lack of significant ongoing star formation, although there is some visible evidence of greenish and blue hues on its exterior edges. The galaxy is likely a mature system that has undergone significant evolution. There is no obvious evidence of a recent major merger event, although some minor gravitational disturbance cannot be ruled out based on this image alone.
