  Using one archival high dispersion high quality spectrum of HR 7098 (A0V)
obtained with the \'echelle spectrograph SOPHIE at Observatoire de Haute
Provence, we show that this star is not a superficially normal A0V star as
hitherto thought. The model atmosphere and spectrum synthesis modeling of the
spectrum of HR 7098 reveals real departures of its abundances from the solar
composition. We report here on our first determinations of the elemental
abundances of 35 elements in the atmosphere of HR 7098. Helium and Carbon are
underabundant whereas the very heavy elements are overabundant in HR 7098.
