In spiral galaxies, integrated optical spectra of NSCs show that they nearly always have multiple stellar populations [@walcher06; @rossa06]. More specifically, NSCs typically have a young stellar population ($<$100 Myr) but are dominated in mass by stars older than $>$1 Gyr. Further support to this picture comes from the observations of several distinct populations in the color-magnitude diagram of the nucleus of the Sgr dwarf spheroidal [M54; @monaco05; @siegel07]. In @seth06 (Paper I), we found from a study of edge-on galaxies that in some NSCs these multiple stellar populations appear to be associated with different morphological components. These clusters are flattened along the major-axis of the galaxy and have color maps and morphologies that suggest they consist of young disks and older more spheroidal components.

We present here follow-up observations of the NSC in NGC 4244, the nearest galaxy in the Paper I sample [D=4.3 Mpc, 1$\arcsec$=21 pc; @seth05a]. In Paper I, we presented integrated optical spectra of this cluster that indicate the presence of multiple stellar populations. Although the detailed star formation history is not well-constrained, populations of 50-100 Myr combined with older populations are required to provide a good fit to the spectra. Redshifted emission identified with an 