The galaxy presents as a slightly elongated, elliptical structure. It exhibits a concentrated central bulge that transitions into a diffuse halo. The core region displays a yellowish-orange hue. This suggests a population of older stars. Fainter, cooler redder regions appear within the central bulge. The outer regions of the galaxy are less defined, fading gradually into the background. The smooth appearance supports its classification as an elliptical galaxy. The overall color profile indicates a lack of significant recent star formation.
