The galaxy presents as a single, somewhat elliptical object. It exhibits a smooth light distribution with a central concentration that brightens significantly towards the core. There is very little visual evidence of substructure, such as spiral arms or dust lanes. The galaxy's color is distinctly redder than the surrounding background, implying a population of older stars. There is no evidence of a strong tidal interaction or any morphological peculiarities, such as a warped disk or extended tidal tails, suggesting it has not undergone a recent major merger. Based on its overall appearance, the galaxy is likely an early-type galaxy, either an elliptical or lenticular galaxy, consistent with a spheroid-dominated system. There may be some minor disturbances present, but the galaxy is mostly undisturbed.
