The galaxy exhibits a clear spiral structure, demonstrating well-defined arms extending from a central bulge. The arms appear loosely wound, showcasing active star formation regions, identifiable by their distinct bluish color. These regions suggest the presence of numerous young, hot stars. The dust lanes are visible within the spiral arms, appearing as dark, obscuring bands. The central bulge exhibits a yellowish hue, indicative of an older stellar population. The overall color suggests the galaxy is actively forming stars with a high star formation rate. There is an apparent asymmetry of the spiral arms, with some disturbances, suggesting a minor gravitational interaction or merger event in its recent past. The galaxy is not seen edge-on, but at an angle. A weak bar structure may be present across the central region.
