This galaxy exhibits a prominent, albeit somewhat diffuse, spiral structure. The arms are well-defined, displaying a moderate to tight winding pattern as they emanate from the central region. A substantial portion of the galaxy's light is concentrated within these spiral arms, which appear somewhat flocculent. Within these arms, there is evidence of active star formation regions, indicated by the presence of bright blue concentrations. The central bulge appears relatively small. There is a suggestion of a bar-like structure extending across the galaxy's core, however it is not particularly strong. There may be some disturbance evident within the morphology of the galaxy, but no other mergers or additional major disturbances are visually confirmed.
