The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The core region exhibits a bright, yellowish-white hue, indicating an older stellar population. The isophotes appear relatively regular. The galaxy displays a slight elongation, deviating from a perfect circular shape. Fainter, bluer light extends from the central bulge into a diffuse halo or disk component. There appears to be a subtle disturbance or asymmetry in the outer regions on one side, potentially indicative of a minor interaction or tidal feature, though the overall structure remains largely undisturbed. The galaxy appears relatively isolated in the image, with no obvious major companion galaxies or signs of a recent major merger event.
