The galaxy presents a flattened, disk-like morphology, suggestive of a spiral or lenticular type. A central bulge is clearly visible, exhibiting a concentrated, bright luminosity, possibly indicating a high density of stars within the galactic nucleus. The light from the bulge appears yellowish-white.

Surrounding the central bulge, fainter, bluer light is apparent extending outward. This potentially indicates the presence of a galactic disk with ongoing star formation. The disk appears to have some patchiness in the distribution of light, though defined spiral arms are not clearly delineated.

There is an indication of some minor disturbances to the disk structure. It may be undergoing minor interactions or accretion events. The elongation of the galaxy is moderate, appearing to be in between a circular and cigar shape.
