The galaxy presents as a flattened, disk-like structure viewed nearly edge-on from our perspective. The central region exhibits a pronounced bulge, appearing as a concentrated region of relatively smooth, yellowish-white light. This suggests an older stellar population dominates the nuclear region. Fainter material extends away from the central bulge in a thin disk, which seems to be a combination of white and light blue, possibly indicating active star formation. There's not any apparent substructure, such as spiral arms or prominent dust lanes visible. The galaxy appears relatively isolated with no nearby companions visibly interacting with it. The disk presents as smooth overall, lacking intense star forming regions.
