The galaxy presents as an elliptical morphology. The central bulge is prominent, exhibiting a concentrated, bright yellowish-white hue indicative of an older stellar population. The outer regions display a fainter, more diffuse halo with a slightly bluer tint, suggesting the presence of some younger stars or ongoing, but limited, star formation activity. The galaxy appears relatively undisturbed, lacking any obvious signs of recent major mergers or tidal interactions. The overall structure suggests a galaxy that has largely completed its morphological transformation toward a more quiescent state.
