This galaxy exhibits a distinct spiral structure, although somewhat flocculent in appearance. The arms are not sharply defined but rather appear patchy and irregular, suggesting ongoing or recent star formation activity. These arms appear to emanate from a moderately sized central bulge, which seems to be relatively smooth and concentrated. The overall color of the galaxy appears bluish, indicative of a younger stellar population, especially within the spiral arms.

There is evidence of possible interactions or disturbances. The asymmetry in the arm structure and some tidal features suggest that this galaxy is undergoing or has recently undergone a minor merger. Some areas appear brighter, possibly due to areas of increased star formation activity, while others are fainter, indicative of older stellar populations or dust obscuration. The spiral arms display a winding morphology.
