The galaxy appears as an elliptical or lenticular type, characterized by a smooth, centrally concentrated light distribution. There is little evidence of spiral arms or significant dust lanes. The core region is bright and yellowish-white, suggesting a population of older stars. The outer regions appear to have a slightly more reddish hue. There is a faint surrounding halo or envelope visible, though it is not extensive. Based on its apparent smoothness and lack of defined structure, it is likely an evolved system. There are no obvious signs of ongoing major merger activity, though a slight asymmetry may suggest minor disturbances.
