geometry is significantly more extended in the K-band, but its size is quite sensitive to the fitted value of the background.

Based on disk fits to the full galaxy from 2MASS presented in @seth05a, the central luminosity surface density of the NSC is $\sim$250$\times$ greater than that of the disk, while the luminosity surface density at the edge of the NIFS field is comparable to the level predicted by the galaxy disk model. Deprojecting the disk components, the luminosity volume density at the center of the NSC is $\sim$10$^6\times$ that of the underlying galaxy disk. The local volume density of the cluster thus dominates the mass in the central regions of the galaxy out to the edge of our data.

[lcccc]{}

\
& $\mu_0$ \[L$_\odot$/pc$^2$\] & $h_x$ \[pc\] & $z_0$ \[pc\] &\
K-band [**disk**]{}$+$Sérsic & 1.4$\times$10$^5$ & 3.39 & 1.19 &\
K-band [**disk**]{}$+$King & 1.9$\times$10$^5$ & 2.72 & 1.38 &\
F814W [**disk**]{}$+$King & 9.7$\times$10$^4$ & 2.73 & 1.42 &\
\
& $\mu_0$ \[L$_\odot$/pc$^2$\] & $r_{eff}$ \[pc\] & $(b/a)$ &\
K-band disk$+$[**King**]{} & 4.5$\times$10$^4$ & 13.6 & 0.79 &\
F814W disk$+$[**King**]{} & 5.3$\times$10$^4$ & 5.70 & 0.73 &\
& $\mu_{eff}$ \[L$_\odot$/pc$^2$\] & $r_{eff}$ \[pc\] & $(b/a)$ & $n$\
K-band disk$+$[**Sérsic**]{} & 