This galaxy presents as a spiral type. It exhibits a discernible disk structure with spiral arms. The spiral arms appear somewhat flocculent. Two dominant arms are most clearly visible. A bulge is present, contributing to the overall luminosity. A bar structure is present, although it is not the dominant feature of the galaxy's morphology. There is no sign of a major merger event, or any major disturbance. The spiral arms appear to have a medium winding.
