The galaxy displays a pronounced spiral structure. The spiral arms appear somewhat tightly wound and are moderately defined. It is difficult to ascertain a precise count, but the galaxy appears to exhibit a multi-armed spiral structure, likely three or four arms, with moderate symmetry. There is evidence of significant star formation within the arms, with a diffuse, patchy appearance. The central bulge appears relatively small compared to the overall galactic disk, with a smooth appearance. The galaxy is generally face-on, offering a clear view of its disk. The absence of a strong bar structure is noted. There are no obvious signs of a major ongoing merger, however, there are some visual disturbances that may indicate a minor interaction. Overall, it appears to be a relatively normal spiral galaxy, with moderate star formation activity.
