The galaxy appears to be undergoing a significant merger event. At least two distinct galactic nuclei are visible, one with a bright, relatively concentrated core and a somewhat diffuse halo, and another that is smaller in apparent size with a more compact, intense core. The overall morphology is heavily disturbed, showing evidence of tidal interactions and possible star formation regions, with a notable fraction of the galaxy appearing to be involved in this merger. There is some indication of a bridge of material connecting the two primary components. The overall color suggests a range of stellar populations, from older, redder stars to younger, bluer stars concentrated in areas of active star formation. The light is strongly distributed towards the redder wavelengths.
