Thrymr is about 8 kilometres in diameter, and orbits Saturn at an average distance of 20,810 Mm in 1120.809 days. It may have formed from debris knocked offPhoebe. The Thrymian orbit isretrograde, at aninclination of 175° to theecliptic (151° to Saturn's equator) and with aneccentricity of 0.453.[3] LikeIjiraq andKiviuq, Thrymr's orbit overlaps strongly with Phoebe's such that it is likely to collide with it in the future.[4]
Its rotation period is38.79±0.25 hours, the slowest among the retrograde moons measured byCassini–Huygens and the second-slowest afterTarqeq.[3] Having two maxima and two minima in itslight curve, it may therefore be acontact binary, although this is less likely than for Kiviuq andBestla.[4] The surface of Thrymr is gray in color and similar to those ofSuttungr andMundilfari, suggesting a common origin as fragments knocked off of Phoebe early in the Solar System's history.[4] In particular, it may be part of the same dynamical family as Suttungr, thoughS/2004 S 7 is probably more closely related.[4]