This galaxy exhibits an elliptical morphology, appearing largely smooth and rounded in shape. There is a strong indication of an ongoing or recent interaction or merger event based on the distorted form. The galaxy presents as a single core with a less distinct secondary core, the two are separated by a less bright region of the galaxy. The overall color profile is predominantly yellow, suggesting a population of older stars. The intensity of the light suggests it is a galaxy of significant mass. The observed features indicate that it has little to no star formation present.