The galaxy presents a distinct spiral structure, with two prominent arms that appear somewhat tightly wound. There is evidence of ongoing star formation within these arms, indicated by subtle blue concentrations. A bar structure is visibly bisecting the galaxy's core and extending along a good portion of the galaxy's total diameter. The galaxy exhibits a noticeable bulge that appears moderate in size relative to the disk. There is a slight disturbance in the disk morphology, indicating a possible interaction or recent minor merger event. Overall, it appears to be a typical spiral galaxy with ongoing star formation and a noticeable bulge and bar.
