The galaxy presents a spiral morphology with a prominent disk structure. The spiral arms appear somewhat tightly wound and are visible extending from a central bulge region. A moderate-sized bulge is present. The color suggests active star formation is occurring within the spiral arms. There's no obvious presence of a strong central bar. Some mild disturbance of the galaxy's structure is apparent. No strong signs of an ongoing merger are seen, but some interaction cannot be ruled out. The inclination is such that we see the galaxy mostly face-on.
