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Using Chandra data, we searched for a pulsar wind nebula (PWN) and found evidence of extended emission in a 3.5-15 arcsec annulus around the pulsar, with a luminosity $L_{\\rm 0.5-8\\,keV}^{\\rm ext} \\sim 8\\times 10^{28}$ erg s$^{-1}$ (at the distance of 288 pc), which is a fraction of $\\sim 0.05$ of the non-thermal pulsar luminosity. 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