This galaxy appears to be undergoing a significant interaction, possibly a merger. The system exhibits a complex morphology with a significant amount of tidal disturbance. Two distinct nuclei are visible, each possessing a relatively bright, compact core. A faint, diffuse stellar bridge or tidal tail stretches between these cores, indicating gravitational interaction. While one core is fairly compact, the other seems to be more disfigured, with signs of starburst activity occurring around it. Star formation seems to be fairly high in this galaxy, due to the blue light scattered around the edges of the galaxy, but further data would be needed to determine the SFR. Overall, this interacting system suggests a dynamic environment likely triggering elevated star formation.
