The galaxy presents as a concentrated, centrally bright object, likely an elliptical or lenticular type. Its light profile appears smooth, lacking any significant spiral arm structures or prominent dust lanes. The core region exhibits a yellowish-orange hue, suggesting a population of older stars. There's a faint, diffuse halo extending outwards from the central bulge. Based on the observed morphology, the galaxy seems relatively undisturbed, with no obvious signs of recent major mergers or tidal interactions. 
