The galaxy appears to be undergoing a significant merger event. The primary visual characteristic is the presence of two distinct, bright nuclei, suggesting two galaxies in the process of coalescing. Tidal features or extended diffuse light surrounding the central regions are not readily apparent in the image, indicating that the merger is possibly in its earlier stages.

The object exhibits spiral structure. The presence of these features and their color suggest ongoing star formation activity within the disk. A central bulge is visible, appearing to be of moderate size relative to the disk. Evidence of a strong central bar is lacking, with only hints of a weak bar-like structure.

The galaxy's overall morphology is complex, resulting from the interaction. It is exhibiting a significant degree of interaction/merging, with disk features beginning to be disrupted or distorted.
