This galaxy exhibits characteristics suggesting an ongoing or recent interaction. There's evidence of tidal disturbances, with extended and distorted features indicating possible merging activity. The galaxy core appears relatively smooth and rounded but is surrounded by fainter, disturbed regions. Within this disturbed area, there are several concentrated knots of light, possibly regions of active star formation triggered by the interaction. Overall, the galaxy presents a complex morphology indicative of a system undergoing gravitational interaction.
