The galaxy presents as a system of interacting or merging galaxies. One galaxy appears nearly edge-on, exhibiting a flattened disk morphology. It displays some irregular light distributions, potentially indicative of tidal interactions. Another nearby galaxy is more face-on and appears to have a smooth and round morphology, but is visibly disturbed. Evidence of possible tidal tails or bridges is present. The overall color of the system is moderately blue, suggesting a population of relatively young stars and ongoing star formation. The morphology appears to be disrupted from interactions with another galaxy.
