[14] The family is old, about (3±1)×109 years, and located near the 3:1 resonant region with Jupiter that supplies near-Earth objects to the inner Solar System.
[14]: 23 In February 2012, a rotational lightcurve of Schürer was obtained from photometric observations by an international collaboration under the lead of South Korean astronomers.
Lightcurve analysis gave a rotation period of 6.66±0.05 hours with a brightness amplitude of 0.77 magnitude, indicative of an elongated, non-spherical shape (U=3-).
It gave a similar sidereal period of 6.5119±0.0002 hours, as well as a spin axis at (235.0°, −26.0°) in ecliptic coordinates (λ, β).
[9] The Collaborative Asteroid Lightcurve Link assumes an albedo of 0.21 and calculates a diameter of 11.55 kilometers based on an absolute magnitude of 12.0.