The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears largely spheroidal, with a gradual decrease in luminosity from the core to the outer regions. There is little to no evidence of spiral arms, prominent dust lanes, or other distinct features typically associated with disk galaxies. The color profile suggests a population of older stars, with a yellowish-red hue dominating the central bulge. The outer regions show a slightly bluer tint, potentially indicative of some younger star formation but this could also be due to imaging artifacts. A faint, diffuse halo may be present, extending slightly beyond the main body of the galaxy. There is no obvious sign of ongoing major mergers or tidal disturbances, although subtle asymmetries could indicate minor interactions in the past.
