The galaxy appears to be in a late-stage merger. It is comprised of two primary luminous components. The northern component exhibits a bluer color, suggestive of ongoing or recent star formation. The southern component appears more yellow/red, possibly indicating an older stellar population or significant dust obscuration. There is some tidal debris visible between the two components. The overall morphology is highly disturbed, lacking a clear spiral or elliptical structure. There are no obvious spiral arm features. It appears relatively compact, though the tidal features hint at a larger, fainter extended halo.
