This galaxy exhibits a clear spiral structure, with two well-defined arms extending from a central region. The arms are somewhat loosely wound, displaying a medium-pitch angle. Star formation is evident within the spiral arms, indicated by the presence of numerous blue regions, likely HII regions. These areas suggest active star formation.

The galaxy's bulge is of moderate size relative to the disk, not dominating the overall structure. There is no obvious bar structure present, or only a very weak one. The disk is not edge-on; it is seen at an angle that allows its spiral structure to be clearly observed.

Evidence suggests that this galaxy is undergoing a merger or experiencing a major disturbance. Tidal features or distorted morphology are visible, indicating interaction with another galaxy. This interaction has produced significant changes in the structure.
