The comparison of the CKM mixing angles with the leptonic mixings implied b
y the recent atmospheric and solar neutrino data exhibits an interesting co
mplementarity. This pattern can be understood in the context of the SU(5) g
rand unification, assuming that the fermion mass matrices have Fritzsch-lik
e structures but are not necessarily symmetric. (The present contribution i
s based on the paper in ref. [1].)