The electroweak (EW) sector of the Minimal Supersymmetric Standard Model (MSSM), with the lightest neutralino as Dark Matter (DM) candidate, can account for a variety of experimental data. This includes the DM content of the universe, DM direct detection limits, EW SUSY searches at the LHC and in particular the so far persistent 3 − 4 σ discrepancy between the experimental result for the anomalous magnetic moment of the muon, (g − 2) µ , and its Standard Model (SM) prediction. The recently published "MUON G-2" result is within 0.8 σ in agreement with the older BNL result on (g − 2) µ . The combination of the two results was given as a exp µ = (11659206.1 ± 4.1) × 10 −10 , yielding a new deviation from the SM prediction of ∆a µ = (25.1 ± 5.9) × 10 −10 , corresponding to 4.2 σ. Using this improved bound we update the results presented in Ref. [1] and set new upper limits on the allowed parameters space of the EW sector of the MSSM. We find that with the new (g − 2) µ result the upper limits on the (next-to-) lightest SUSY particle are in the same ballpark as previously, yielding updated upper limits on these masses of ∼ 600 GeV. In this way, a clear target is confirmed for future (HL-)LHC EW searches, as well as for future high-energy e + e − colliders, such as the ILC or CLIC.