The galaxy presents as a somewhat elongated structure. It appears to be undergoing a merger or interaction, as evidenced by the disturbed morphology and the possible presence of tidal features. The main body is a diffuse elliptical component with a central bright region. Some redder patches are visible, possibly indicating regions of dust obscuration or older stellar populations. The overall color is relatively uniform, suggesting an evolved stellar population and modest star formation. The galaxy appears to be of substantial size and mass. There are some indications of a potential bar-like structure across the center.
