This galaxy appears to be in the process of a major merger or is exhibiting significant tidal disturbances. The system consists of at least two distinct luminous components. One component appears more spheroidal and has a yellowish color, potentially indicating an older stellar population or significant dust obscuration. The second component is more elongated, possibly a disrupted disk, and also exhibits a yellowish hue, although it appears to have some bluer, possibly star-forming regions. There is evidence of a bridge or tail-like structure connecting or emanating from these components. This overall morphology suggests an ongoing or recent gravitational interaction that has significantly disrupted the original structures of the galaxies involved.
