The galaxy presents as a somewhat diffuse, centrally concentrated object. Its color appears relatively uniform and moderately red-shifted. No distinct spiral arms or bar structures are discernible within the galaxy's morphology. The shape is largely elliptical, but not perfectly so. Evidence suggests it may be undergoing a minor merger event or has experienced some gravitational disturbance, which can be seen as a slight irregularity in the shape of the galaxy. There may be a small population of young stars forming.