Two absorption line indices, Ca II and H delta/lambda 4045, measured from h
igh-resolution spectra are used with evolutionary synthesis models to verif
y the presence of a young stellar population in NGC 5018. The derived age o
f this population is similar to 2.8 Gyr with a metallicity roughly solar, a
nd it completely dominates the integrated light of the galaxy near 4000 Ang
strom.