The galaxy in the image exhibits a distinct spiral structure. The spiral arms are clearly visible, with a tightly wound morphology in some parts and a more open, loosely wound structure in others. The arms appear somewhat flocculent. There appears to be a dominant population of blue stars in the spiral arms, suggesting active star formation.

The galaxy's disk is observed nearly face-on. A central bulge is present, although it appears relatively small in comparison to the overall disk size. There is no obvious bar-like structure transecting the bulge.

There are potential signs of gravitational interactions or minor disturbances, such as subtle distortions in the outer spiral arms. However, there is no strong evidence of a major merger event based on this image alone.
