The galaxy exhibits a clear spiral structure. The spiral arms appear tightly wound around a central bulge region, though the bulge itself is not particularly prominent. There is no evidence of the galaxy being edge-on; it is presented at an angle closer to face-on. The spiral arms are somewhat flocculent, displaying a patchy distribution of light, and feature notable concentrations of bright, potentially young, stellar populations, indicated by their bluish color. There is no obvious central bar structure bisecting the bulge region. The galaxy appears relatively isolated, showing no signs of major ongoing mergers or significant tidal disturbances, although some minor irregularities are visible. The spiral arms continue to trail off into a haze further and further from the center. Overall, the galaxy appears as a fairly typical spiral galaxy with moderate star formation occurring within its arms.
