The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. There is no apparent disk structure or spiral arm features visible. The light is generally diffuse, displaying a radial gradient decreasing from the bright core. The color profile suggests a population of older stars, with redder hues in the outer regions and a slightly bluer, possibly younger stellar population toward the center. The galaxy appears relatively undisturbed, without signs of major mergers or significant tidal interactions. There is a very slight asymmetry in the outer halo, though this could be caused by background objects or noise. The round shape and lack of noticeable dust lanes supports its classification as an elliptical galaxy.
