The galaxy presents as a centrally concentrated, relatively smooth object. The morphology appears primarily elliptical or spheroidal. A distinct, bright central bulge or core region is observed, showing a yellowish hue, possibly indicating an older stellar population. Moving outward from the core, the galaxy exhibits a gradual decrease in luminosity, with a diffuse halo that extends outwards. There's a hint of a flattened shape; however, no prominent spiral arm structures or dust lanes are discernible in the image. The outer regions display subtle color variations, with a slight bluer tint compared to the central core, potentially indicating the presence of younger stars or star-forming regions in the outer disk. Overall, the galaxy seems to be relatively undisturbed, lacking obvious signs of major mergers or significant tidal interactions, though minor disturbances cannot be ruled out.
