SED fits to photometry of the putative host cluster of SN 1994W. The combined magnitude of both the point source and any diffuse emission is shown at the wavelength of each band. SED models have been scaled to match the F606W band, and are plotted in red. We see that populations with log(Age) between 6.0 and 6.6 dex match, with the exception of the F336W band, while the older 6.8 dex population does not match either the F450W or the F814W band.