The galaxy presents a clear spiral structure, with well-defined arms emanating from a central, moderately sized bulge. The spiral arms exhibit a tightly wound morphology. There is strong evidence of significant star formation activity concentrated within the spiral arms as indicated by the clumpy and blue hue. This suggests a population of young, massive stars. Dust lanes are also possibly present, though not distinctly visible. The disc is viewed close to face on, providing a clear view of its spiral structure. There is no obvious major disturbance or signs of a recent major merger event. The image indicates the galaxy's light is dominated by the disk and spiral arms.
