The galaxy presents as a spiral type, exhibiting prominent spiral arm structures. The arms appear somewhat disrupted, suggesting possible interactions or internal disturbances. The central bulge region is moderately sized and displays a yellowish hue, indicative of an older stellar population. A prominent bar structure is visible bisecting the bulge, and its morphology suggests it is on the stronger side. There appears to be a companion galaxy interacting with the main galaxy, thus further explaining the distorted arms and its overall merging nature.

Overall, the galaxy shows signs of active star formation, particularly within the spiral arms, as indicated by the patchy blue regions. Its edge is not visible, suggesting we are seeing it face on. The disk is fairly well defined.