The galaxy presents as a generally smooth, elliptical morphology, with a high degree of central concentration. The luminosity profile appears to gradually decrease from a bright, yellowish core outwards. There is little to no evidence of spiral arm structure or distinct disk features, though there is a very slight indication of bluer light on one side. Overall, the galaxy appears relatively undisturbed, exhibiting no significant signs of major mergers or tidal interactions with other galaxies. The light is somewhat redder in the central regions and slightly bluer in the outskirts.
