The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The core region exhibits a high surface brightness, gradually diminishing outwards into a more diffuse halo. There is a slight blue tint in the outer regions and a yellow center, suggestive of a potential difference in stellar populations, with possible ongoing or recent star formation in the periphery and older stars in the core. The overall structure appears largely undisturbed, lacking any obvious signs of recent major mergers or tidal interactions.
