The galaxy appears to be undergoing a significant interaction, possibly a merger. The morphology is highly disturbed, with a dominant, seemingly spheroidal component and a prominent, elongated tidal tail extending outwards. The primary component exhibits a relatively smooth profile. The tail displays a color gradient, appearing bluer at the leading edge, suggesting recent star formation, and redder as it merges with the body of the galaxy. Overall, the system exhibits a dynamic and evolving state, indicative of a gravitational interaction.
