The galaxy exhibits a clear spiral structure, observed at an intermediate inclination. Two spiral arms appear dominant. The arms are relatively loosely wound, with a flocculent, patchy structure. A distinct central bulge is observed, exhibiting a more concentrated luminosity. The bulge color appears yellowish-white, indicative of an older stellar population. Blue hues are observed in the spiral arms, suggesting ongoing star formation. There is a faint hint of a bar-like structure extending through the center of the bulge, but it is weakly defined. Overall, this appears to be a disk galaxy with clear spiral features.
