The galaxy presents as a spiral, seen at a slight inclination. Two prominent spiral arms are visible, winding moderately around the central bulge. The bulge appears relatively small compared to the overall disk size. A potential bar structure seems to traverse the galaxy's center. Star formation is occurring, as indicated by the clumpy, patchy regions within the spiral arms. There is no visually apparent evidence of any major mergers or significant disturbances of the disk.
