The galaxy presents as an elliptical, spheroid-dominated system. It exhibits a smooth, centrally concentrated light profile, lacking any discernible spiral arms or significant disk-like features. The color gradient suggests an older stellar population, particularly in the core, with the redder hues indicating a prevalence of evolved stars. The outer regions appear slightly bluer, hinting at the presence of some younger stars, but the overall color is relatively uniform. There is no strong evidence of active star formation regions or prominent dust lanes within the galaxy. The galaxy appears relatively undisturbed, showing no clear signs of recent mergers or tidal interactions. The morphology aligns with an early-type galaxy classification.
