The galaxy exhibits a merging or interacting morphology. There appear to be two distinct components. The first component, in the northern region, is relatively smooth and round, with a concentrated, bright core. The second component, located in the southern region, is larger and more diffuse, with a less-defined core. A bridge of diffuse light connects the two components, suggesting tidal interactions and material exchange between them. Overall, the galaxy shows signs of significant gravitational disturbance, likely due to the ongoing merger process.
