  We present $N$--body models for triaxial elliptical galaxies or halos of
galaxies, which are fully self--gravitating, have near constant axis ratio as a
function of radius and a $r^{-1}$ central density cusp. Preliminary
investigation suggests the model are stable and orbit analysis shows no
indication of chaotic orbits. The models provide a starting point for
investigations into the evolution of triaxial figures of equilibrium, response
of triaxial figures to central black holes, external perturbations and
interactions.
