The galaxy exhibits a spiral morphology with a disk structure. Spiral arms are visible, extending outward from a central region. The galaxy appears somewhat face-on, allowing for a clear view of its overall structure. The bulge is not very large, and there appears to be no bar feature. There is evidence of some ongoing star formation activity. The galaxy does not appear to be undergoing any major merging events, but shows some signs of minor disturbances to its morphology. The color is biased towards the blue end of the spectrum, especially at the outer edges of the galaxy.
