The galaxy presents a distinctly featured morphology, dominated by spiral arm structures. These arms exhibit a predominantly tight winding pattern. While difficult to ascertain an exact count, several spiral arms are suggested. A prominent but not dominant bulge component is observed, contributing significantly to the overall galactic luminosity. The galactic disk is viewed face-on, and exhibits no signs of being an edge-on disk. There is no obvious indication of merging activity. The galaxy is of moderate size.
