  We re-investigate UZ Librae spectra obtained at KPNO in 1998 and 2000. From
the 1998 data we compose 11 consecutive Doppler images using the Ca I-6439, Fe
I-6393 and Fe I-6411 lines. Applying the method of average cross-correlation of
contiguous Doppler images we find anti-solar differential rotation with a
surface shear of alpha ~ -0.03. The pilot application of the local correlation
tracking technique for the same data qualitatively confirms this result and
indicates complex flow pattern on the stellar surface. From the
cross-correlation of the two available Doppler images in 2000 we also get
anti-solar differential rotation but with a much weaker shear of alpha ~
-0.004.
