The galaxy presents as a spiral structure, exhibiting prominent spiral arms. These arms are relatively tightly wound around a distinct central bulge. The bulge appears moderately sized. A bar-like structure seems to exist extending from the central bulge, possibly weak in nature. The overall color of the galaxy suggests active star formation, evidenced by the bluer hues within the spiral arms. There is no obvious indication of a major merger event. Some disturbance can be seen within the body of the galaxy.
