The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The core region appears bright and yellowish, suggesting a population of older stars. Surrounding this central region is a more diffuse halo of light, exhibiting a reddish tint, possibly indicating the presence of dust or a population of cooler stars. The overall structure appears relatively undisturbed, without any obvious signs of tidal interactions or major mergers. The shape is generally round, with a slight elongation. There is no clear evidence of a prominent disk or spiral arms. Overall, the galaxy appears to be a relatively evolved system, likely a massive elliptical galaxy with limited ongoing star formation.
