  We present a novel approach for simultaneous extraction of stellar population
parameters and internal kinematics from the spectra integrated along a line of
sight. We fit a template spectrum into an observed one in a pixel space using a
non-linear $\chi^2$ minimization in the multidimensional parameter space,
including characteristics of the line-of-sight velocity distribution (LOSVD)
and parametrized star formation history (SFH). Our technique has been applied
to IFU and multi-object spectroscopy of low-luminosity early type galaxies.
