The galaxy appears to be undergoing a significant interaction or merger event. The main body presents a relatively smooth, elliptical morphology with a bright, concentrated nucleus. Extending away from the main body, there is a distinct tidal tail or stream of diffuse material. This feature suggests gravitational disruption due to a past or ongoing interaction. There is a noticeable asymmetry in the overall structure, with the tidal feature being more prominent on one side. The color gradients within the galaxy suggest varying stellar populations and dust content, with bluer regions potentially indicating areas of more recent star formation, possibly triggered by the interaction. Overall, the morphology indicates a complex system influenced by gravitational interactions, potentially with another galaxy or a smaller satellite galaxy.
