The galaxy appears to be a lenticular or early-type spiral galaxy, potentially at an intermediate stage of morphological transformation. The galaxy exhibits a central, relatively bright bulge with a smooth texture. The bulge appears elongated and potentially somewhat bar-shaped. It is characterized by a red-shifted color, possibly indicating an older stellar population. Fainter, bluish components extend outwards from the central bulge. These components are less defined, but suggest the presence of a disk. The galaxy’s overall shape can be described as moderately elongated, not perfectly round, with a hint of a disk-like structure. There is evidence of minor disturbances or asymmetries in the disk, with hints of possible tidal interactions or merging events. These disturbances could be contributing to the galaxy's current morphology. It is likely undergoing some sort of merging or tidal interaction with a smaller companion galaxy.
