The galaxy presents a largely smooth and symmetrical morphology. It appears elliptical in shape, exhibiting a gradual increase in luminosity towards a bright central region which likely hosts a supermassive black hole. The light profile suggests a well-defined core, with a diffuse halo extending outwards. There's a subtle color gradient, transitioning from a yellowish-white core to a slightly redder outer region. No distinct spiral arms or bar structures are discernible. The overall structure suggests a relatively evolved system with a substantial stellar mass. There is no apparent tidal disruption or interactions with nearby galaxies.
