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We report the results of high-resolution ($R \sim 80,000$) spectroscopicobservations of the emission-line object HD 85567, which has been classified asa FS CMa type object or a pre-main-sequence star. The main goal is to put moreconstraints on the object's fundamental parameters as well as on its nature andevolutionary state. Absorption lines in the spectrum of HD 85567 were foundsimilar to those of mid B--type dwarfs and correspond to the followingfundamental parameters: T$_{\rm eff} = 15000\pm500$ K, $v \sin i = 31\pm3$ kms$^{-1}$, $\log g \sim 4.0$. The interstellar extinction, A$_V$ $= 0.50\pm0.02$mag, was measured using the strengths of some diffuse interstellar bands. Wealso obtained $UBV(RI)_{\rm c}$ images of a $10^{\prime} \times 10^{\prime}$region around the object. Photometry of projectionally close stars was used toderive an interstellar extinction law in this direction and resulted in adistance of 1300$\pm$100 pc to the object and a luminosity of $\log$(L/L$_\odot) = 3.3\pm0.2$. We found no significant radial velocity variationsof the absorption lines in the spectra of HD 85567 obtained during twomonth-long periods of time in 2012 and 2015. Our analysis of the spectroscopicand photometric data available for the star led us to a conclusion that itcannot be a pre-main-sequence Herbig Ae/Be star. We argue that thecircumstellar gas and dust were produced during the object's evolution as mostlikely a binary system, which contains an undetected secondary component and isunlikely to be a merger product.

Towards Understanding The B[e] Phenomenon: VI. Nature and Spectral Variations of HD 85567