for the optical data (see Paper I, Fig. 4), a single component elliptical King (or Sérsic) profile fit to the K-band image leaves behind significant residuals in the plane of the galaxy. Combined with the optical color difference (Fig. \[popfig\] top panel), this motivates us to fit the data using both a spheroidal [*and*]{} disk component. All models were convolved by a Gaussian PSF with FWHM of 0.23$\arcsec$ during the fitting process. We tried both disk$+$King (as used in Paper I) and a disk$+$Sérsic profile. Both profiles provide fits with reduced $\chi^2$ values $\sim$4$\times$ smaller than the spheroidal component alone. The values of the derived parameters for these fits, and the disk$+$King F814W filter fit from Paper I, are shown in Table \[fittable\]. The parameters for the disk fits are the central surface brightnesss $\mu_0$, the scale length $h_x$, and scale height $z_0$. For the spheroidal component fits, the parameters are the central surface brightness $\mu_0$ (King) or effective surface brightness $\mu_{eff}$ (Sérsic), effective radius $r_{eff}$, axial ratio $(b/a)$, and Sérsic index $n$. The derived K-band disk sizes are very similar to those derived at optical wavelengths from the HST data despite the lower resolution of this data. The spheroid 