 The body's observation arc begins with its official discovery observation at Palomar in March 1983.Although "George" is a member of the dynamical Hungaria group, it is not a member of the collisional Hungaria family but an unrelated, non-family asteroid from the background population, according to Nesvorý, Milani and Knežević.However, in a 2014-abstract from the "Asteroids, Comets, Meteors Conference" in Helsinki (ACM 2014), "George" was mentioned as the principal body of a newly discovered low-density family in the Hungaria region.