The galaxy presents as a relatively small, edge-on spiral system. A distinct dust lane bisects the galaxy's disk, running along its major axis and obscuring some of the starlight. The bulge is not particularly prominent, appearing somewhat diffuse and elongated along the disk. The spiral arms are not well-defined, suggesting a flocculent or weakly structured morphology. The overall color of the disk appears blueish, indicative of ongoing star formation. The galaxy shows no obvious signs of major interaction or merging events, although some minor disturbances are difficult to rule out at this resolution. There is a faint satellite galaxy or star cluster that can be seen on the upper left side of the disk.
