The galaxy presents as a spiral, viewed at a high inclination, bordering on edge-on. Evidence suggests a small bulge is apparent from the concentration of light at the core with spiral arms emerging from the center. The arms appear tightly wound and are somewhat difficult to distinguish due to the inclination. The spiral arms indicate active star formation regions, suggested by their blue hue. The galaxy appears to be experiencing some form of gravitational disturbance or interaction, evidenced by slight asymmetries in the disc and the presence of possible tidal features extending from one end. There may be a bar structure present. The galaxy appears relatively smooth, without signs of major ongoing merger activity beyond the disturbances already noted.
