  The kinematics, structure, and stellar population properties in the centers
of two early-type spiral galaxies of the Leo Triplet, NGC 3623 and NGC 3627,
are studied by means of integral-field spectroscopy. Unlike our previous
targets, NGC 3384/NGC 3368 in the Leo I group and NGC 5574/NGC 5576 in LGG379,
NGC 3623 and NGC 3627 do not appear to experience a synchronous evolution. The
mean ages of their circumnuclear stellar populations are quite different, and
the magnesium overabundance of the nucleus in NGC 3627 is evidence for a very
brief last star formation event 1 Gyr ago whereas the evolution of the central
part of NGC 3623 looks more quiescent. In the center of NGC 3627 we observe
noticeable gas radial motions, and the stars and the ionized gas in the center
of NGC 3623 demonstrate more or less stable rotation. However, NGC 3623 has a
chemically distinct core -- a relic of a past star formation burst -- which is
shaped as a compact, dynamically cold stellar disk with a radius of about
250-350 pc which has been formed not later than 5 Gyr ago.
