The few known \gamma -ray binary systems are all associated with variable radio and X-ray emission . The TeV source HESS J0632 + 057 , apparently associated with the Be star MWC 148 , is plausibly a new member of this class . Following the identification of a variable X-ray counterpart to the TeV source we conducted GMRT and VLA observations in June-September 2008 to search for the radio counterpart of this object . A point-like radio source at the position of the star is detected in both 1280 MHz GMRT and 5 GHz VLA observations , with an average spectral index , \alpha , of \sim 0.6 . In the VLA data there is significant flux variability on \sim month timescales around the mean flux density of \approx 0.3 mJy . These radio properties ( and the overall spectral energy distribution ) are consistent with an interpretation of HESS J0632 + 057 as a lower power analogue of the established \gamma -ray binary systems .