The galaxy presents an irregular morphology, appearing to be in the late stages of a major merger event. The system exhibits two distinct luminous cores, one with a bluer spectral signature and the other more redshifted, possibly indicating differences in stellar population or dust obscuration. The overall shape is highly disturbed, lacking a well-defined disk or spiral arms. There are tidal features or extended plumes of stellar material visibly connecting the two nuclei, implying strong gravitational interactions. The system appears to be relatively compact, given the bright absolute magnitudes. The rate of star formation is likely suppressed due to the late stage merger. The presence of morphological disturbance suggests that the galaxy has undergone a significant transformation from its original form.
