This galaxy exhibits a prominent disk structure, not quite edge-on, with a clearly defined central bulge. The bulge appears to be of moderate size, showing a yellow to white color, indicative of an older stellar population. Spiral arms are evident, though somewhat tightly wound around the bulge, making the exact count difficult to discern. There is a hint of blue color in the outer regions of the disk, which may be due to younger stars. The galaxy appears to be relatively isolated, with no obvious signs of major interactions or mergers occurring, though some minor disturbances or asymmetries are not ruled out. There may be a weak bar structure, but the resolution limits the ability to confirm.
