The galaxy appears to be a relatively bright, centrally concentrated object. It exhibits a smooth, elliptical morphology with a high degree of roundness, showing minimal features indicative of spiral arms or prominent dust lanes. The central bulge region is characterized by a yellowish-white hue, potentially indicating an older stellar population. The outer regions of the galaxy gradually fade into the background, displaying a slightly more reddish tint. There are no obvious signs of major tidal disturbances or interactions with other galaxies, and the overall structure suggests a relatively undisturbed system.
