This galaxy presents as a face-on spiral, exhibiting a well-defined disk structure. The spiral arms are prominent, tightly wound around a central bulge. The bulge appears relatively small in comparison to the overall disk size. A faint bar structure may exist, though it is not strongly pronounced. The spiral arms show a mottled texture, indicative of areas of active star formation. The color distribution suggests a mix of stellar populations, with bluer regions concentrated in the spiral arms, likely regions of young, hot stars, and a yellower hue in the bulge, potentially indicating an older stellar population. The overall morphology suggests a galaxy undergoing active star formation within its spiral arms, with a relatively quiescent bulge region. The galaxy does not show any obvious signs of major merger activity, though minor disturbances cannot be ruled out. Dust lanes appear intertwined within the spiral arms, contributing to the patchy appearance. There are more than four spiral arms.