The galaxy exhibits a predominantly smooth morphology. The central region displays a high concentration of light, appearing as a bright, relatively uniform core. There is a faint, diffuse halo extending outwards from the central core, though its boundaries are somewhat irregular and asymmetric. A slight elongation is discernible, but the overall shape is generally round. Color gradients within the galaxy suggest a possible presence of younger stellar populations closer to the core. The galaxy appears relatively isolated, showing no obvious signs of major interaction with other galaxies or large disturbances. Faint structural features or tidal tails are not readily apparent. There is the possibility of a minor merger or disturbances based on the overall shape.
