The galaxy presents a flattened, disk-like morphology, viewed nearly edge-on. A prominent dust lane bisects the galaxy, visible as a dark band against the brighter stellar population. The central bulge is somewhat obscured by the dust lane, but appears to be relatively small. The galaxy exhibits a distinct blue color in its outer regions suggesting ongoing star formation, particularly along the edges of the disk. Fainter, diffuse light extends above and below the primary plane of the galaxy, potentially representing a halo of older stars or scattered light. No signs of strong tidal interactions or major mergers are apparent, although there might be a hint of minor disturbance in the disk structure. The overall appearance suggests a spiral or lenticular galaxy at a moderate redshift.
