This galaxy appears to be in the late stages of a major merger event. There are two distinct, bright nuclei, indicating the centers of the progenitor galaxies have not yet fully coalesced. The overall shape is highly disturbed and irregular, lacking a well-defined disk or spiral structure. There is a noticeable tidal tail emanating from one of the galactic nuclei, hinting at strong gravitational interactions. The galaxy exhibits a somewhat smooth appearance, however closer inspection may reveal pockets of ongoing star formation. Overall, this object likely has a substantial stellar mass and modest star formation rate for its mass.
