The galaxy exhibits a spiral morphology, appearing face-on relative to our line of sight. It displays well-defined spiral arms that wind tightly around a central bulge. The bulge appears relatively small and not particularly luminous compared to the rest of the galaxy. A bar structure is either not present or very weak. The spiral arms are prominent and show a complex structure, with regions of varying brightness possibly indicating areas of active star formation. There is no obvious evidence of a major ongoing merger, although some subtle disturbances or asymmetries in the outer regions could suggest a past interaction or minor disturbance. The overall color suggests a mix of stellar populations, with bluer regions in the spiral arms indicative of younger, hotter stars and redder hues closer to the bulge suggesting older stellar populations. Many spiral arms are present, more than four.
