This galaxy exhibits a prominent, relatively bright central bulge. Surrounding the bulge, there are clear spiral arm structures extending outwards. The arms appear somewhat fragmented and asymmetric, with one arm appearing more diffuse than the other. The bluer hues observed within the spiral arms suggest ongoing star formation. There is a possible disturbance to the galactic structure, indicated by the asymmetry in the arms and general morphology, hinting at possible gravitational interaction with another galaxy. The spiral arms have moderate winding and appear primarily as one or two defined arms. There is no clear presence of a strong bar structure. The overall shape of the galaxy could be classified as a spiral galaxy that is not edge on.
