The galaxy presents as a somewhat diffuse object with an elliptical morphology. It exhibits a smooth overall appearance, with a primary concentration of light and a secondary concentration of light. The color is notably redder than the surrounding field, suggesting an older stellar population or significant dust obscuration. There is a possibility that the light concentration is not due to an interaction, but is instead simply two cores due to an older merger. There is a possible minor disturbance in the object's core but it is difficult to make a definitive evaluation.
