The galaxy presents a smooth, elliptical morphology. It exhibits a centrally concentrated bulge with a gradual decrease in luminosity extending outwards. The overall color profile suggests a dominant population of older stars, with a slightly redder hue in the central regions and a subtle bluer tinge towards the outer edges. There is no clear evidence of spiral arms or significant dust lanes. The galaxy appears relatively undisturbed, lacking any obvious signs of recent merger activity or tidal features.
