This galaxy exhibits a generally smooth, elliptical morphology. The core is a bright, concentrated region, displaying a yellowish-white hue, which likely indicates a population of older stars. Moving outwards from the core, the galaxy fades into a more diffuse, greenish halo. There's also a slight reddening in the outer regions, possibly signifying areas of dust or a population of cooler stars. No distinct spiral arms or bar structures are visible. There is no apparent presence of any major mergers or tidal disturbances.
