The galaxy exhibits a distinct spiral structure, although somewhat disrupted. The spiral arms appear loosely wound and asymmetric, with two dominant arms clearly visible. There is evidence of ongoing interaction or a merger event; the morphology shows significant disturbance.

The central bulge appears moderate in size and displays a yellowish-white hue, indicative of an older stellar population. A bar-like structure may be present, but it is difficult to confirm, and if present, it is not prominently defined.

Extensive blue regions are present along the spiral arms, suggesting active star formation. There are also reddish regions that could represent dust lanes within the galaxy. The overall color of the galaxy is predominantly blue-white, indicating a mix of stellar populations. There appears to be a considerable amount of tidal debris and potential merging companions at the bottom.
