The galaxy presents a largely smooth, elliptical morphology with minimal visible substructure. The central region exhibits a high surface brightness, appearing as a concentrated, yellowish-white core that suggests an older stellar population. The light gradually diminishes outwards from the core, extending into a diffuse halo. There is a subtle color gradient present, shifting from a warmer, yellower hue at the core to a slightly bluer tone in the outer regions, potentially indicating the presence of younger stars in the outer halo. There is no apparent spiral structure or distinct dust lanes discernible in the image. The overall form indicates a system that has undergone significant dynamical relaxation. There is no evidence of major recent mergers or tidal disturbances.
