The galaxy models are the same shape parameters in all filters, which does not allow for color gradients. We could capture color gradients by allowing the bulge and disk fluxes (for composite galaxies) to freely float relative to one another. This would probably be dangerous to do with something like the DR1 reductions, where these effects are likely small when compared to the remaining systematics in the PSF mis-estimation.
The galaxy models are the same shape parameters in all filters, which does not allow for color gradients. We could capture color gradients by allowing the bulge and disk fluxes (for composite galaxies) to freely float relative to one another. This would probably be dangerous to do with something like the DR1 reductions, where these effects are likely small when compared to the remaining systematics in the PSF mis-estimation.