The galaxy appears as a centrally concentrated, roughly circular object with a smooth light profile. The central region exhibits a bright, yellowish-white hue, indicative of an older stellar population. There is a subtle gradient in color and brightness extending outwards from the core. The outer regions fade into a dimmer, slightly bluer halo, suggesting the presence of some younger stars. The overall morphology suggests a classification as an early-type galaxy, potentially an elliptical. There is no visible evidence of spiral arms, distinct features, or significant tidal disturbances. The galaxy appears to be a relatively isolated system with no obvious signs of recent or ongoing merger activity.
