Wolf-Rayet stars represent a final stage of evolution for massive stars, where they have lost their outer atmosphere due to either binary interactions or through stellar winds. As such, direct measurements of stellar masses are an ideal way to test stellar/binary evolution. To date, only a few carbon-rich Wolf-Rayet stars have resolved orbits through long-baseline optical interferometry. We present the first results on WR133 (WN5 + O9I) with the CHARA Array. We resolved the binary (P=112 d) in July 2019 with the MIRCX combiner, with a separation of 0.9 mas, moving about 2-3 degrees per day. We have collected three more snapshots since the discovery and will present a preliminary orbit, constrained by a previously published spectroscopic orbit this January at the AAS meeting.