  We report the first-ever discovery of an extragalactic Wolf-Rayet (WR)star
with Spitzer. A new WR star in the Large Magellanic Cloud (LMC) was revealed
via detection of its circumstellar shell using 24 {\mu}m images obtained in the
framework of the Spitzer Survey of the Large Magellanic Cloud (SAGE-LMC).
Subsequent spectroscopic bservations with the Gemini South resolved the central
star in two components, one of which is a WN3b+abs star, while the second one
is a B0V star. We consider the lopsided brightness distribution over the
circumstellar shell as an indication that the WR star is a runaway and use this
interpretation to identify a possible parent cluster of the star.
