This galaxy exhibits a pronounced disk structure, though it is not perfectly edge-on. It appears to be a spiral galaxy, based on the presence of arm-like features extending from the central bulge. The spiral arms appear tightly wound around the central bulge. While difficult to precisely quantify, the spiral arms seem to be numerous. The central bulge is relatively small. There is no evidence of a strong bar feature bisecting the central region. The disk shows some signs of disturbance but does not appear to be undergoing a major merger. The galaxy is dominated by blue light, meaning there could be significant star formation activity present. There is a small red area on the edge of the galaxy. 
