The galaxy exhibits an elongated morphology. The central region presents a concentrated luminosity profile, appearing relatively smooth. There is a faint extension of diffuse light emanating from the core. The overall color appears bluish, which may be caused by ongoing star formation. There is a possible tidal tail or disruption on one side of the galaxy. There is a very faint disk structure. It may be undergoing a merger. The galaxy displays a mixture of smooth and featured characteristics.
