The galaxy presents a somewhat elliptical morphology, appearing more elongated than perfectly spherical. The central region exhibits a high concentration of light, suggesting a prominent galactic nucleus or bulge. The luminosity gradually decreases from the center outwards. There are hints of spiral structure, but they are not well-defined or prominent. The overall color appears relatively redder, potentially indicating an older stellar population or significant dust content. The galaxy seems relatively undisturbed, without any major morphological distortions suggesting recent or ongoing mergers, however there could be minor disturbances. The roundness appears to be somewhat between round and cigar shaped. Overall, the galaxy appears to be a relatively massive and old galaxy, with possible evidence of on going star formation.
