The galaxy appears as an elliptical-like structure with a bright, concentrated central bulge. There is little visible structure suggesting spiral arms or a distinct disk, indicating a relatively smooth morphology. The galaxy exhibits a color gradient, with the central bulge appearing more yellow/red and the outer regions possessing a slightly bluer tint. This color distribution could indicate an older stellar population concentrated in the core with some ongoing, but low, star formation in the outer areas. The overall roundness and lack of obvious tidal features suggests no recent major mergers or significant gravitational disturbances. The galaxy appears relatively undisturbed.
