The galaxy presents a smooth, elliptical morphology. It exhibits a centrally concentrated bulge, appearing nearly spherical and dominating the overall structure. The light profile smoothly decreases outwards from the core. There is a faint, diffuse halo of light surrounding the central region, gradually blending into the background sky. No distinct spiral arms or prominent dust lanes are discernible within the resolution of the image. The color profile appears homogenous across the galaxy, with a slight reddening towards the core suggesting a population of older stars. There are no obvious signs of recent or ongoing major mergers or tidal disturbances. The galaxy appears relatively undisturbed and isolated.
