The galaxy exhibits a distinct spiral morphology. The spiral arms appear loosely wound, suggesting a relatively late-type spiral galaxy. The arm structure is somewhat flocculent, lacking the grand design seen in some other spirals. From what can be seen, there appears to be a single dominant spiral arm. The central bulge of the galaxy is moderately sized, taking up approximately 57% of the galaxy's volume. It is neither particularly prominent nor exceptionally faint. There is no evidence for a strong central bar structure; if present, it is weak. There is a considerable amount of disturbance in the galaxy, including a possible minor merging event. The overall appearance is bluish, indicative of ongoing star formation within the spiral arms. The galaxy is not observed edge-on.
