The galaxy appears to be a relatively smooth, elliptical-type system, exhibiting a centrally concentrated luminosity profile. The core region presents a yellowish-white hue, suggesting an older stellar population. The outer regions of the galaxy are slightly more diffuse and exhibit a faint bluish tint, which could indicate the presence of some younger, hotter stars or ongoing, low-level star formation. The galaxy appears largely undisturbed, with no obvious signs of tidal interactions or recent major mergers. The overall morphology suggests a system in a relatively late stage of its evolution, with ongoing but subdued star formation. The galaxy's shape is generally round.
