The galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a distinct yellowish-red hue, possibly indicating an older stellar population and/or dust obscuration. Extending outward from the center is a more diffuse region with a greenish tint, suggesting the presence of some younger stars. There is a subtle disk-like structure visible at the edges. The galaxy appears largely undisturbed, lacking major signs of tidal interactions or ongoing mergers. Its overall morphology is consistent with an evolved system, with a dominance of older stellar populations and a relatively low rate of star formation.
