This galaxy presents as a somewhat edge-on spiral with a high degree of asymmetry. One side of the galaxy appears extended, with a greater observed length. The core region displays a slight central bulge, with a flattened disk extending outwards. The overall color of the galaxy appears to be a blue-green hue, hinting at ongoing star formation, particularly in the disk. The disk itself exhibits some clumpy regions, potentially indicative of active star-forming regions or spiral arm structures, although the resolution limits precise determination. There are subtle signs of possible tidal disturbances or interactions, suggesting a past or ongoing minor merger event. The disk of the galaxy appears to be warped or distorted, possibly due to gravitational interactions. There is no prominent central dust lane, but a faint, uneven absorption band can be seen, consistent with the presence of dust clouds within the galaxy.
