We present theBBXRTspectrum of the black hole candidate LMC X‐1. The spectrum cannot be fit by a simple model, but requires a soft disk blackbody component and a power law tail, confirming earlier studies. The blackbody disk component is essentially unchanged since theGingameasurement in 1987. We report a 95% confidence detection of weak emission features at ∼5.1 keV and ∼7.3 keV; if attributed to Fe I K&agr; at 6.39 keV, when the redshift is ∼0.19. No quasi‐periodic behavior is found in the data at this epoch. ©1994 American Institute of Physics.