The galaxy presents as a spiral with a moderate inclination. Traces of spiral arms can be observed extending outward from a central bulge. The bulge appears to be of moderate size relative to the galactic disk and exhibits a smooth texture.

The overall color profile of the galaxy suggests ongoing star formation, particularly within the spiral arms, indicated by the presence of bluer hues. The central bulge appears more yellow. The galactic disk appears to have some clumpy structures.

The galaxy is unlikely to be undergoing a major merger, though there are some irregularities that suggest possible minor disturbances to its structure.
