The ISO and IUE spectra of the elliptical nebulae NGC7662 and NGC6741 are p
resented. These spectra are combined with the spectra in the visual wavelen
gth region to obtain a complete, extinction corrected, spectrum. The chemic
al composition of the nebulae is then calculated and compared to previous d
eterminations. The abundances found are compared to determinations made in
other nebulae using ISO data. A discussion is given to see if possible evol
utionary effects can be found from the abundance differences.