The galaxy presents a generally elliptical morphology. It exhibits a smooth, diffuse light distribution with a notable concentration towards the center. The core region appears significantly brighter and takes on a yellow-orange hue, potentially indicating an older stellar population or a concentration of dust. Fainter, bluer light surrounds the central region extending outwards to form the more diffuse edges of the galaxy. There is no apparent disk structure or spiral arm morphology evident in this observation. Overall, the galaxy appears relatively undisturbed, exhibiting no signs of ongoing major mergers or tidal distortions.
