The galaxy presents as a spiral type, exhibiting a central bulge that appears moderate in size. The spiral arms are prominent, with a clear winding pattern of moderate tightness. The disk is viewed nearly face-on, with little indication of an edge-on orientation. There is a subtle blueish tint along one side of the disk, suggestive of ongoing star formation regions. There are disturbances in the morphology of the disk indicating a possible merger. The overall structure displays noticeable features rather than a smooth, elliptical profile.
