Notes.—Col. (1) galaxy name. Col. (2) morphological classification from RC3 (de Vaucouleurs et al. 1991). Col. (3) while distance (D) are primarily from the NASA/IPAC Extragalactic Database NED (3K CMB), other sources are Karachentsev et al. (2004, k) and Bonanos et al. (2006), (b). Col. (4) optical spectral class from Baldi et al. (2021a): H II, L = LINER, S = Seyfert, and ALG = Absorption Line Galaxy. ‘RL’ indicates radio loud galaxies (Baldi et al. 2021b). Col. (5) the central velocity dispersion (σ) from Ho et al. (2009). Cols. (6)-(8) V-band bulge, nucleus, and galaxy magnitudes calculated by integrating the best-fit Sérsic, Gaussian, or core-Sérsic functions and applying our colour transformation equations listed in Table 4 (see Section 3.3). Cols. (9) the stellar mass-to-light ratios (M/L) measured in the HST bands listed in Tables B.2−B.4. Cols. (10-12) we did not convert the V-band magnitudes into stellar masses, instead the luminosities of the bulge, nucleus, and the galaxy measured in the HST bands (listed in Tables B.2−B.4) were converted into stellar masses (M_*) using our M/L values (col. 9). Cols. (13) logarithm of the SMBH mass (M_BH) for galaxies with measured M_BH from van den Bosch (2016), except for NGC 205 which is from Nguyen et al. (2019). The BH masses are adjusted here to our distance. Col. (14) logarithm of the 1.5 GHz radio core luminosity (L_R, core). Col. (15) average ellipticity of the bulge inside R_e omitting PSF-affected region (< ϵ> ). Col. (16) median of the isophote shape parameter inside R_e (Med (B₄)). Col. (17) inner logarithmic slope of the bulge light profile. Col. (18) radio detection of the galaxies are based on Baldi et al. (2021a) and following their nomenclature ‘I’ = detected and core identified; ‘unI?’ = detected but core unidentified; ‘U’ = undetected; ‘I+unI?’ = detected and core identified having additional unknown source(s) in the FOV. The full table is available at the CDS.