The galaxy presents as a flattened, disk-like structure when viewed from our perspective. A bright central bulge is present, surrounded by what appears to be a prominent disk. There seems to be a feature running through the disk that gives the impression of a ring surrounding the central bulge. There are subtle color variations within the disk, which could indicate differing stellar populations or dust lane obscuration. The faint outer regions surrounding the galaxy appears smooth, possibly indicating a large halo of older stars or diffuse gas. Overall, the morphology does not suggest a strong presence of significant merging activity.
