The galaxy presents as a disk galaxy, viewed at an oblique angle. It exhibits a prominent central bulge, appearing moderately bright, and an extended, fainter disk. The disk shows hints of spiral structure, though it appears somewhat flocculent. There's a slightly off-center, secondary body of light which could be another galaxy or a region of star formation. Dust lanes are subtly visible within the disk, running along the near side of the galaxy relative to our line of sight, indicating some degree of interstellar medium obscuration. The galaxy shows an overall blueish tint, potentially suggesting active star formation. The shape is elongated, implying a high inclination angle with respect to the observer.
