The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a bright, somewhat diffuse core region that fades into an extended, less luminous halo. The overall shape appears generally elliptical, with a moderate degree of roundness. There is no clear evidence of spiral arm structures or significant dust lanes. Slight asymmetry in the outer halo might suggest past minor interaction, but is not definitively indicative of a major merger event. The color gradient appears relatively uniform across the galaxy, with a slightly redder hue in the central regions, suggesting a potentially older stellar population in that area.
