The galaxy appears as a centrally concentrated object with a smooth overall morphology. It exhibits a bright, compact core that gradually fades into a more diffuse halo. The shape is predominantly round, showing no strong evidence of a disk or spiral structure in the visible light. There is no indication of any major mergers or significant disturbances affecting the overall galactic structure. Subtle color gradients are observable, with the central region appearing slightly yellower compared to the outer regions, which show hints of a bluer hue. Overall, the galaxy presents as a relatively undisturbed, evolved system.
