LS 5039 is a massive x-ray binary with persistent radio emission at a distance of 3.1 kpc. Recent high resolution radio observations with the VLBA reveal that LS 5039 is resolved into bipolar jets emanting from a central core, revealing its microquasar nature. This system also appears to be associated with the EGRET source 3EG J1824-1514. The association with the $\gamma$-ray source is further supported by LS 5039 being the only bright x-ray and radio source within the EGRET 95% confidence contour.