This galaxy exhibits a largely elliptical morphology, displaying a smooth, centrally concentrated light profile. The galaxy's core is relatively bright, with a gradual decrease in luminosity observed towards its outer regions. There is no obvious disk structure, nor spiral arm features present in the image. The galaxy appears to be relatively undisturbed with no indication of any tidal tails, or prominent distortions indicating a recent major merger event. Its overall color index indicates an older stellar population, with a relative absence of young, blue stars. There are no indications of active star formation regions present. Based on its morphology and the presence of older stars, this is likely to be a relatively massive galaxy.
