The galaxy presents as a relatively smooth, elliptical or lenticular structure. The light is concentrated towards the center, with a diffuse halo extending outwards. There's a subtle color gradient, with a slightly bluer tint in the outer regions and a more yellowish hue toward the core, hinting at different stellar populations and potential star formation activity. The overall symmetry suggests a mature system without signs of recent major mergers or significant tidal disturbances, with only minor perturbations and few if any disks. There is no bar structure or spiral arms that can be seen. The galaxy’s shape is generally round with slight variation.
