We show that the horizon geometry for supersymmetric black hole solutions of minimal five-dimensional gauged supergravity is that of a particular Einstein-Cartan-Weyl (ECW) structure in three dimensions, involving the trace and traceless part of both torsion and nonmetricity, and obeying some precise constraints. In the limit of zero cosmological constant, the set of nonlinear partial differential equations characterizing this ECW structure reduces correctly to that of a hyper-CR Einstein-Weyl structure in the Gauduchon gauge, which was shown by Dunajski, Gutowski and Sabra to be the horizon geometry in the ungauged BPS case. * dietmar.klemm@mi.infn.it † lucrezia.ravera@mi.infn.it 1 In four dimensions, one can have black holes with nonspherical horizons by relaxing some of the assumptions that go into Hawking's theorem. For instance, in asymptotically anti-de Sitter (aAdS) space, the horizon of a black hole can be a compact Riemann surface Σ g of any genus g [3], or a sphere with two punctures [4,5]. In the latter case, the horizon is noncompact but has yet finite area. For aAdS spaces, both the asymptotically flat and dominant energy conditions are violated.