The galaxy appears as a relatively bright, disk-shaped structure. There is evidence of spiral arms, though not sharply defined, displaying a somewhat flocculent or patchy appearance. A central bulge is visible, exhibiting a smoother, more concentrated light distribution than the surrounding disk. The blue color of the galaxy suggests ongoing star formation. The galaxy is not perfectly symmetrical, showing some indication of possible gravitational interaction or minor disturbances. The galaxy is relatively compact, not showing extended or diffuse features. Overall, it appears as a spiral galaxy with moderate star formation activity.
