The galaxy presents as a barred spiral, exhibiting a distinct central bulge that is subtly elongated along the bar structure. This bar extends approximately across half the diameter of the visible galaxy. The spiral arms are prominent, although somewhat tightly wound, displaying a patchy distribution of star-forming regions indicated by bluish hues along their length. The disk component dominates the overall structure, with a relatively small bulge in comparison. The galaxy is viewed at an oblique angle, but not edge-on. The galaxy has a relatively high inclination. There are no signs of any recent major merger event, or any major disturbances.
