The galaxy presents a disk-like morphology. Distinct spiral arm structures are visible, with the arms appearing somewhat loosely wound. A central bulge is present, though it appears to be relatively small in proportion to the overall disk size. The galactic disk exhibits patchy regions of blue light, suggestive of ongoing star formation. There are also hints of a possible bar structure in the center. The galaxy may be experiencing minor gravitational interactions, or possibly a merger with a smaller galaxy based on the slightly disturbed structure of its spiral arms.
