The galaxy presents as a spiral type, with a prominent, moderately sized central bulge that appears relatively bright and concentrated. From the overall morphology, the galaxy is viewed at an oblique angle, not quite face-on but also not edge-on, allowing for some spiral arm structure to be visible. 

The spiral arms are somewhat loosely wound and show a patchy distribution of light, potentially indicative of active star formation regions. A bar-like structure seems to be present traversing the central bulge. The color gradients within the spiral arms suggest a mix of stellar populations, with bluer regions hinting at younger, hotter stars and redder regions potentially containing older, cooler stars or dust. The disk extends a fair distance away from the central bulge, though the edges of the disk are rather faint. There is a moderate presence of HII regions. Some minor disturbances appear to be present in the galaxy's morphology. 
