This galaxy exhibits a morphology suggestive of ongoing gravitational interaction or tidal disturbance. The core region appears relatively smooth and centrally concentrated, emitting a somewhat bluish light. Extending from this central region are faint, diffuse structures hinting at distorted spiral arms or tidal tails. These outer features display a less defined shape, possibly a result of gravitational forces from a nearby galaxy. Overall, the galaxy appears to be undergoing a merging or interaction process, where it is experiencing disturbances in its outer structure. The galaxy does not appear to have a defined disk-like structure. 
