The galaxy presents as a centrally concentrated, relatively smooth elliptical structure. The core appears bright and slightly reddish. Moving outward from the core, there is a gradual decrease in luminosity, with a more diffuse, bluish halo surrounding the central region. No distinct spiral arms or bar structures are discernible. There is very little evidence of tidal disturbances or interactions with other galaxies in the immediate vicinity. The overall morphology suggests a mature galaxy, potentially with a population of older stars dominating its stellar content.
