  We report the results of our search for the progenitor candidate of SN
2013dk, a Type Ic supernova (SN) that exploded in the Antennae Galaxy system.
We compare pre-explosion Hubble Space Telescope (HST) archival images with SN
images obtained using adaptive optics at the ESO Very Large Telescope. We
isolate the SN position to within 3 sigma uncertainty radius of 0.02", and show
that there is no detectable point source in any of the HST filter images within
the error circle. We set an upper limit to the absolute magnitude of the
progenitor to be M_F555W > -5.7, which does not allow Wolf-Rayet (WR) star
progenitors to be ruled out. A bright source appears 0.17" away, which is
either a single bright supergiant or compact cluster, given its absolute
magnitude of M_F555W=-9.02 +- 0.28 extended wings and complex environment.
However, even if this is a cluster, the spatial displacement of SN 2013dk means
that its membership is not assured. The strongest statement we can make is that
in the immediate environment of SN 2013dk (within 10 pc or so) we find no clear
evidence of either a point source coincident with the SN or a young stellar
cluster that could host a massive WR progenitor.
