S/2004 S 24 is about 3 kilometres in diameter, and orbits Saturn at an average distance of 22.901 Gm in 1294.25 days, at an inclination of 35.5° to the ecliptic, in a prograde direction and with an eccentricity of 0.085.[1] Due to its inclination being similar to members of the Gallic group, S/2004 S 24 could belong to the Gallic group.[4] However, its orbit is much more distant, which puts this classification into question. It could very well be in a group of its own.
The exact formation mechanism of S/2004 S 24 is unknown, and due to its low eccentricity (0.085) a captured orbit is unlikely. Nonetheless, S/2004 S 24 orbits in the opposite direction of all other moons in its orbital region, making it unlikely to have survived in this orbit over the entire history of the Solar System.
^ abcdeSheppard, Scott. "Scott S. Sheppard - Saturn Moons". Department of Terrestrial Magnetism. Carnegie Institution for Science. Retrieved 7 October 2019.
^ ab"M.P.C. 117075"(PDF). Minor Planet Circular. Minor Planet Center. 10 October 2019.