 In the Bus–Binzel SMASS classification, "Toni" is an X-type asteroid, while in the Tholen classification, it is closest to a common, carbonaceous C-type asteroid and somewhat similar to an X-type (CX).In July 2014, a rotational lightcurve of "Toni" was obtained from photometric observations by Frederick Pilcher at the Organ Mesa Observatory in New Mexico.Lightcurve analysis gave a well-defined rotation period of hours with a brightness amplitude of magnitude ().