The galaxy appears as a relatively smooth, centrally concentrated object. It exhibits an elliptical morphology, with a high degree of roundness. The light distribution indicates minimal presence of spiral arms or a distinct disk-like structure. There is a subtle color gradient, transitioning from a yellowish-orange core to a slightly bluer, more diffuse halo. There is no visual evidence of major ongoing mergers or significant tidal disturbances, although a possible minor interaction or faint feature in the outskirts cannot be ruled out. Overall, the galaxy presents itself as a evolved and relatively undisturbed system.
