The galaxy presents as a relatively smooth, elliptical-like structure, with a primarily yellowish-orange hue. There is some suggestion of a very subtle disk-like component, although the overall morphology is dominated by a bulge-like central region. The overall shape appears to be somewhere between round and elongated, with the potential for being more disc-like. There is no obvious evidence of major mergers or significant tidal disturbances. The color suggests a population of older stars and reduced levels of current star formation. The absolute magnitude indicates a moderately luminous galaxy. Based on its color, the galaxy is likely a fairly massive system with minimal star formation occurring.
