(90568) 2004 GV9 (provisional designation 2004 GV9) is a trans-Neptunian object that was discovered on April 13, 2004 by NEAT.

It has been observed forty-seven times, with precovery images back to 1954.

[9] A diameter of 680±34 km has been determined from combined observations of the Herschel and Spitzer space telescopes.

[10] However, its low albedo suggests it has never been resurfaced and thus is unlikely to have planetary geology.

This article about a centaur (minor planet) or trans-Neptunian object is a stub.