This galaxy appears to be undergoing a major merger, with evidence of significant gravitational disturbance. There seem to be three relatively distinct concentrations of light, potentially representing the cores of the merging galaxies or regions of enhanced star formation triggered by the interaction. The overall shape is elongated and irregular, deviating significantly from a smooth elliptical or well-defined spiral structure. There is some indication of tidal tails or extended diffuse emission surrounding the galaxy. Based on its color, star formation may be present within the system. The central region seems to host a more evolved stellar population, while the outer regions possibly contain younger, bluer stars.
