It's all a matter of scale.
"The core of the Sun is considered to extend from the center to about 20–25% of the solar radius. It has a density of up to 150 g/cm
3"
http://en.wikipedia.org/wiki/Sun
radius = 6.96E+010 cm
core radius = 1.39E+010 cm
core volume = 1.13E+031 cm
3
density = 100 g/cm
3
mass = 1.13E+033 g
percent H = 50.00%
moles H = 5.65E+032 mol
avogadro's number = 6.02E+023
H atoms = 3.40E+056
Stars in both galaxies = 1.00E+012
ratio atoms in sun's core to stars in galaxies = 3.40E+044
Obviously there's a lot of estimating there. But, even if they are all off by an order of magnitude there is still many times more atoms in a star than stars in a galaxy.