The galaxy presents as a spiral type, observed at an inclined angle relative to our line of sight. The central bulge is prominent and appears yellowish-white. The spiral arms are distinct and appear to originate close to the central bulge. The arms are tightly wound around the central bulge. There appear to be two main spiral arms. There may be the presence of a bar feature in the center of the bulge. There is no evidence of a major merger in the system. The spiral arms appear somewhat smooth.