The galaxy presents as a primarily smooth, elliptical-like structure. The central region exhibits a high concentration of light, appearing as a bright yellowish-white core. The light intensity diminishes gradually from the core outwards, forming a halo of diffuse light. There is a subtle indication of a disk-like structure. No distinct spiral arms or bar features are discernible. Overall, the galaxy appears relatively undisturbed, without any major signs of ongoing mergers or tidal interactions, though some minor disturbances cannot be ruled out. It appears to be a relatively massive system with a moderate star formation rate.
