The galaxy appears as a distorted structure, possibly undergoing a merging event. There are two visible nuclei, with one being bluer in color and more compact than the other. The overall morphology suggests significant disruption, with extended tidal features and an irregular shape. The galaxy displays a mix of smooth and irregular features, hinting at both an older stellar population and ongoing or recent star formation activity. There is evidence of dust lanes or obscuration, which may indicate recent merger activity. There are two tidal tails extending from the galaxy. The system exhibits an oblate shape.