The galaxy exhibits a central, concentrated core region that appears relatively smooth and bright. Surrounding the core, there is a more diffuse halo of light. Evidence suggests a subtle disturbance in its overall form. One notable feature is a faint, elongated structure extending outward from the central region, possibly indicative of tidal interactions or past merger events. The galaxy displays an overall flattened shape, suggestive of a disk-like morphology. The distribution of light within the galaxy is not entirely uniform, showing some clumpy regions embedded within the disk. Color gradients are present, with the central regions appearing bluer and the outer halo appearing redder.
