[2] Litva is a member of the Hungaria family, which form the innermost dense concentration of asteroids in the Solar System.
[1] In the Tholen taxonomy, Litva is classified as an EU-type, a subtype of the bright E-type asteroids.
[1] It has also been characterized as a Sl-type and Q-type asteroid by astronomers using the New Technology Telescope at La Silla and by PanSTARRS' photometric survey, respectively.
[10] Most recent photometric observation from 2014, gave a refined period of 2.812186 hours, using a statistical Bayesian inference methodology.
[15] In March 2009 the Central Bureau for Astronomical Telegrams announced the discovery of a moon orbiting the asteroid.