Investigation of gaseous and stellar kinematics and of broad-band VRI and narrow-band H _ { \alpha } and [ NII ] \lambda 6583 images is performed for the central part ( R < 4 kpc ) of the regular spiral galaxy NGC 2841 .
We have found emission-line splitting at R < 20 \arcsec and three-component LOSVD for the stars in the radius range 6 \arcsec \div 100 \arcsec .
Morphological analysis reveals strong narrow shock fronts close to the major axis in the radius range of 30 \arcsec \div 50 \arcsec , a turn of the isophote major axis by 5 \arcdeg and strongly negative Fourier coefficient a _ { 4 } ( boxy isophotes ) in the radius range of 15 \arcsec \div 33 \arcsec .
In principle , all these features may be explained in the frame of a triaxial bulge hypothesis .