The galaxy presents as a moderately luminous, elliptical morphology. It exhibits a smooth, relatively featureless structure with a noticeable central bulge. The galaxy's light profile is centrally concentrated, fading gradually outward from a bright core. The overall color appears slightly red, suggesting a population of older stars. The galaxy is not perfectly spherical, displaying a slightly elongated shape, somewhere in between round and cigar-shaped. No distinct spiral arms or significant dust lanes are discernible. There is no visible evidence of recent major merger activity or strong tidal disturbances. Slight color variation can be seen away from the core, with less-red colors. This could point to some low level star formation in the outer reaches of the galaxy.
