The galaxy appears to be a relatively smooth, elliptical galaxy. Its overall shape is roughly round. The light distribution suggests a centrally concentrated luminosity profile, with a bright, yellowish core gradually fading into a bluer, less luminous halo. There is a slight asymmetry in the outer regions, but no clear signs of spiral arms or a distinct disk. There is no obvious indication of a major ongoing merger or significant tidal disturbances, although some subtle irregularities in the outer halo might suggest minor interactions. The galaxy appears to be moderately massive and undergoing some star formation.
