The galaxy exhibits a prominent spiral structure with arms that are somewhat flocculent. The arms display a mix of winding, ranging from tightly wound to loosely wound segments. There's a notable central bar feature, and it appears quite strong. The bulge is not very prominent; it seems small. Some areas of the galaxy are more disturbed than others. There are segments of the disk that appear to be undergoing some level of merging, or gravitational interaction. Overall, the galaxy exhibits a mix of order and disturbance, which suggests possible ongoing interactions.
