The galaxy appears to be a spiral galaxy, seen at an angle that is close to face-on. The central bulge is bright and moderately sized, indicating the potential for a supermassive black hole. Traces of spiral arm structure are visible, extending from the central bulge outwards. The arms appear somewhat flocculent. There are areas of apparent star formation within the spiral arms, showing bluish regions indicative of younger, hotter stars. The galaxy doesn't appear to be strongly barred. Overall, the galaxy presents a somewhat disturbed morphology, suggesting possible recent interactions or internal dynamical processes.
