The galaxy presents as a centrally concentrated, relatively smooth object with a high degree of symmetry. It appears elliptical in shape, with a bright, concentrated core indicating a substantial central bulge. A diffuse halo extends outwards, with the isophotes becoming somewhat elongated. The color gradient suggests a possible redder population of stars towards the central regions, transitioning to slightly bluer colors in the outer disk, although this difference is subtle. There appears to be little to no evidence of spiral arms or significant dust lanes within the system. The overall visual impression is that of a mature galaxy, with the smooth morphology indicating an older stellar population.
