The galaxy presents as a centrally concentrated, smooth elliptical galaxy. The core exhibits a bright, yellowish-white hue, indicating a population of older stars. The light gradually fades towards the outer regions, transitioning to a slightly redder tone. No distinct spiral arms or dust lanes are apparent within the observed structure. The overall shape appears relatively undisturbed, lacking any signs of major mergers or tidal distortions, though some faint asymmetry on one side indicates a possible minor disturbance. Based on the morphology, the galaxy is likely a massive, quiescent system.
