 In September 2012, a rotational lightcurve of "Wolfiana" was obtained from photometric observations by American astronomers Luis Martinez, Arizona, and Frederick Pilcher at Organ Mesa Observatory (), New Mexico.Lightcurve analysis gave a well-defined rotation period of 4.0654 hours with a brightness amplitude of 0.20 magnitude (), refining a period of 4.0 hours previously measured in November 2009 ().According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, "Wolfiana" measures 8.488 and 8.976 kilometers in diameter and its surface has an albedo of 0.129 and 0.1153, respectively.