The galaxy presents as a largely featureless, smooth object with an approximately elliptical morphology. It is generally round in appearance. The light is centrally concentrated, with a bright, yellowish core that fades into a more diffuse, bluish halo. There is no clear evidence of spiral arm structure or a distinct disk. The galaxy appears relatively isolated, with no obvious signs of ongoing or recent major mergers or tidal disturbances, although there could be minor disturbances present. The color gradient suggests the presence of a relatively older stellar population in the central regions, with potentially younger stars contributing to the bluer outer regions.
