The galaxy presents as a single, luminous entity with a generally elliptical morphology. The light distribution appears centrally concentrated, displaying a smooth gradient outward from a bright core. There is no discernible spiral arm structure or prominent dust lanes. The galaxy exhibits a yellow-white hue, indicative of a stellar population dominated by older, evolved stars. There is no evidence of tidal tails or significant morphological distortions suggesting recent major merger activity, though some minor disturbance is not excluded. Overall, the galaxy appears to be a relatively undisturbed, early-type system.
