helium
hydrogen. its currently fusing hydrogen to helium, but because its a fairly average size star, it will be unable to then fuse the helium into later fuels (carbon, neon, oxygen, silicon). so it expands, sheds off its outer layers and becomes a white dwarf, cooling down until its at ambient temperature as a black dwarf.
Edit: so a sun sized star can use helium as a secondary fuel, fusing it down to carbon after a helium flashover (but thats not where our star is at right now). the resulting white dwarf will be a combination of helium, carbon, oxygen and trace amounts of other elements.