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We present Rc-band surface photometry for 170 of the 203 galaxies in GHASP,Gassendi H-Alpha survey of SPirals, a sample of late-type galaxies for whichhigh-resolution Fabry-Perot H{\alpha} maps have previously been obtained. Ourdata set is constructed by new Rc-band observations taken at the Observatoirede Haute-Provence (OHP), supplemented with Sloan Digital Sky Survey (SDSS)archival data, obtained with the purpose of deriving homogeneous photometricprofiles and parameters. Our results include Rc-band surface brightnessprofiles for 170 galaxies and $ugriz$ profiles for 108 of these objects. Wecatalogue several parameters of general interest for further reference, such astotal magnitude, effective radius and isophotal parameters -- magnitude,position angle, ellipticity and inclination. We also perform a structuraldecomposition of the surface brightness profiles using a multi-component methodin order to separate disks from bulges and bars, and to observe the mainscaling relations involving luminosities, sizes and maximum velocities.  We determine the Rc-band Tully Fisher relation using maximum velocitiesderived solely from H$\alpha$ rotation curves for a sample of 80 galaxies,resulting in a slope of $-8.1 \pm 0.5$, zero point of $-3.0 \pm 1.0$ and anestimated intrinsic scatter of $0.28 \pm 0.07$. We note that, different fromthe TF-relation in the near-infrared derived for the same sample, no change inthe slope of the relation is seen at the low-mass end (for galaxies with$V_{max} < 125$ km/s). We suggest that this different behaviour of the TullyFisher relation (with the optical relation being described by a singlepower-law while the near-infrared by two) may be caused by differences in thestellar mass to light ratio for galaxies with $V_{max} < 125$ km/s.

GHASP: an H$\alpha$ kinematic survey of spiral galaxies - X. Surface photometry, decompositions and the Tully-Fisher relation in the Rc-band