The galaxy presents as a spiral type, exhibiting a disk-like structure with prominent spiral arms. These arms appear tightly wound, originating from a central bulge that is moderate in size relative to the overall galactic disk. The galactic disk shows a clumpy structure. Two spiral arms are observed, however other arms may be too faint to see. The color gradient within the galaxy transitions from a yellowish central bulge, indicating a concentration of older stars, to bluer arms, which are indicative of ongoing star formation. There is no apparent bar structure. No major signs of mergers are present, though the image resolution makes subtle tidal disturbances difficult to resolve.
