The galaxy exhibits a prominent spiral structure. Two distinct spiral arms are visible, tightly wound around the central bulge. The central bulge appears to be of moderate size, contributing a significant portion to the overall light emitted by the galaxy. There is no apparent strong bar structure; the central region appears relatively amorphous. The overall disk is not seen edge-on. Some distortions are observed, suggesting a possible minor disturbance or interaction, but there are no definitive signs of a major merger event.
