The galaxy presents a smooth, elliptical morphology. The light distribution is centrally concentrated, with a gradual decrease in luminosity outwards. The galaxy's color profile suggests a redder central bulge region, potentially indicating an older stellar population. The outer regions appear marginally bluer, possibly indicating ongoing or recent star formation, although this is subtle. There is no apparent evidence of spiral arm structure or a distinct disk. The overall form is regular, showing no obvious signs of major mergers or tidal disturbances. The galaxy's shape appears close to circular.
