The galaxy presents as a centrally concentrated, somewhat elliptical structure. The core region exhibits a yellowish-white hue, suggesting a population of older stars and potentially lower rates of current star formation. There's a gradual transition outwards from this core to a more diffuse, bluer envelope, which might indicate the presence of younger stellar populations at the galaxy's periphery. The overall morphology appears relatively undisturbed, showing no strong signs of recent major mergers or tidal interactions. The galaxy exhibits a smooth appearance with only slight indications of any disk features. There appears to be minimal dust obscuration across the observed light profile.
