The galaxy presents a largely smooth, elliptical morphology, appearing generally rounded in shape. The light distribution exhibits a centrally concentrated profile, fading gradually outwards. The galaxy appears largely undisturbed, with no obvious signs of major mergers or tidal features. There may be some minor disturbances, but it's difficult to tell. Its color suggests a relatively passive stellar population, with older stars dominating the emission. The overall spectral energy distribution suggests moderate to low star formation activity, with a correspondingly high mass.
