The galaxy presents an elliptical morphology, appearing largely smooth and rounded in shape. There are faint, ill-defined spiral arm structures that show very little signs of recent activity. The galaxy possesses a distinct central bulge that shines brighter than the surrounding areas. There are minor distortions of the structure which are likely due to a possible ongoing merger. There is some evidence of active star formation, but this is likely minimal. The overall color index suggests a population of older stars, indicating it is a relatively massive galaxy.