The galaxy presents as a spiral type, showing a prominent disk structure. The spiral arms are clearly visible, winding outward from a central region. The arm structure is somewhat flocculent, appearing patchy and less well-defined in certain regions. There is a suggestion of asymmetry in the spiral arm structure. Star formation appears evident within the arms, indicated by regions of bluer light. The central bulge is not overly prominent. The galaxy does not appear to be undergoing a major merger, although there might be some minor disturbances present in the morphology. The galaxy appears to be viewed at a slight angle relative to face-on.
