The galaxy exhibits a disturbed morphology, suggestive of an ongoing or recent interaction or merger. The light distribution appears to be relatively smooth overall, but with noticeable irregularities. Two brighter, concentrated components are present, likely representing the nuclei of the interacting galaxies or high density star forming areas. There is a tidal tail present that is thin and wispy. The color of the light is generally reddish-yellow, indicating an older stellar population and/or significant dust obscuration. The galaxy does not appear to display a well-defined spiral or elliptical structure. The system is not perfectly circular, with some elongation in its overall shape. The galaxy appears to be in a late stage of merging.
