  We report detection of the binary companion to the millisecond pulsar
J1741+1351 with the Gran Telescopio Canarias. The optical source position
coincides with the pulsar coordinates and its magnitudes are g' = 24.84(5), r'
= 24.38(4) and i' = 24.17(4). Comparison of the data with the white dwarf
evolutionary models shows that the source can be a He-core white dwarf with a
temperature of $\approx 6000$ K and a mass of $\approx 0.2$ M$_{\odot}$. The
latter is in excellent agreement with the companion mass obtained from the
radio timing solution for PSR J1741+1351.
