Kind of an interesting factoid is that Haumea is one of the fastest rotating objects in our solar system.  Here is a bit more on its dimensions and properties:

The first calculations, conducted by Brown et al., provided the approximate dimensions of 2,000 x 1,500 x 1,000 km. Meanwhile, the Spitzer measurements gave it a diameter of 1050 – 1400 km, while subsequent light-curve analyses suggested an equivalent circular diameter of 1,450 km. In 2010 an analysis of measurements taken by Herschel Space Telescope together with the older Spitzer Telescope measurements yielded a new estimate of ~1300 km.

These independent size estimates overlap at an average geometric mean diameter of roughly 1,400 km. In essence, this means that Haumea is comparable in diameter to Pluto along its longest axis and about half that at its poles.  It’s mass, meanwhile, is estimated to be approximately 4.0 ×10²¹ kg – one-third the mass of Pluto and 1/1400th that of Earth.

This makes Haumea one of the largest trans-Neptunian objects discovered, smaller than Eris, Pluto, probably Makemake, and possibly 2007 OR10, but larger than Sedna, Quaoar, and Orcus. Combined with estimates of its density, Haumea is massive enough to have achieved hydrostatic equilibrium. Although Haumea appears to be far from spherical, its ellipsoidal shape is thought to result from its rapid rotation.

Just a note, this dwarf planet also has an unusual dark spot.  Jupiter of course has the large red spot and is in an entirely different class of planet.  We hope you like the video.

thanks to universetoday.com for the great info

thanks to NASA for the pic