The galaxy exhibits a complex morphology, appearing to be undergoing a significant interaction or merging event. Two distinct components are visible. The first component presents a more concentrated, yellowish core, with a roughly elliptical shape. It appears relatively smooth, suggesting a population of older stars. The second component displays a bluer hue and a more diffuse structure. There is evidence of tidal distortion, with extended faint features that point away from the main body of the galaxy, suggesting gravitational disturbance.

Based on the extended light observed around the galaxy, the system is likely dynamically young, and the color variations suggest differences in stellar populations across the interacting components.
