The galaxy exhibits a disturbed morphology, potentially indicative of an ongoing or recent interaction. The primary body of the galaxy appears somewhat rounded, with evidence of tidal features extending outwards. These features suggest gravitational interactions with another galaxy. There appears to be a distinct tidal bridge of material, possibly composed of gas and dust, connecting the primary body to another galaxy.

The colors observed suggest varying stellar populations and dust content throughout the galaxy. Overall, the galaxy shows signs of active star formation, consistent with a system experiencing gravitational interaction.
