The galaxy presents as a single, relatively smooth, centralized light source. The light appears generally symmetric, with an apparent roundness. There is a distinct, brighter core region that may indicate the presence of an active galactic nucleus (AGN) or a concentrated region of stars. The outer regions of the galaxy show a more diffuse glow, fading gradually from the brighter core. There may be a slight hint of a disk-like structure, but the lack of defined spiral arms or other features suggests this galaxy is likely a lenticular or elliptical galaxy. No signs of significant tidal disturbances or ongoing mergers are apparent. The overall color suggests a population of older stars and potentially a lower star formation rate, with a slight hint of younger stars near the center.
