The galaxy presents as a smooth, elliptical morphology. The light profile is centrally concentrated with a diffuse halo, exhibiting a high degree of symmetry. The core region appears bright and slightly yellowish, suggesting a population of older stars. There is no evidence of spiral arms, a prominent disk, or significant dust lanes. The overall color gradient shifts subtly from yellow in the center to a slightly bluer hue in the outer regions, hinting at the presence of a small population of younger stars, though the galaxy is predominantly comprised of an older stellar population. There's no clear evidence of tidal features or ongoing mergers, though the outer regions show some slight asymmetry that could point towards an interaction in the past. The galaxy does not present with strong signs of star formation.
