The galaxy presents a spiral structure, exhibiting a distinct disk with relatively tightly wound spiral arms. The arms appear somewhat flocculent, showing significant star formation activity along their lengths, indicated by a bluer color. The central bulge is prominent, appearing yellowish-white, suggesting an older stellar population. The galaxy exhibits an inclination, appearing almost face-on, which allows for detailed observation of the spiral structure. A weak bar feature seems to be present across the nucleus. The overall morphology suggests a galaxy undergoing active, though not extreme, star formation. There might be some minor tidal disturbances.
