The galaxy presents as a slightly inclined spiral, exhibiting a defined disk structure. Spiral arms are visible, showing a degree of patchiness rather than being fully continuous and smooth. These arms appear somewhat flocculent in nature. The central bulge region is apparent, with a subtle concentration of light, however the bulge is not particularly prominent compared to the disk. There is evidence of blue star formation regions scattered throughout the spiral arms. The galaxy does not show any obvious signs of major mergers. Some irregularities in the outer disk regions might suggest minor gravitational interaction or disturbances. There is a possibility of a weak bar feature present across the central region.