The observed galaxy exhibits a distinct spiral morphology. The central bulge appears prominent and exhibits a yellowish-white hue, suggesting a population of older stars. Fainter spiral arms extend outwards from the bulge, tracing a well-defined disk.

The arms are tightly wound, displaying a relatively continuous structure with hints of flocculent regions. Discontinuities and less well-defined areas within the arms suggest differential rotation.

The overall color of the spiral arms indicates a mixed population of stars. Faint bluer regions indicate more recent and ongoing star formation, while yellower/whiter regions suggest a more evolved population. The galaxy's structure doesn't suggest a major ongoing merger event. The observed features point towards a relatively isolated spiral galaxy undergoing typical evolutionary processes. 
