  We present high-resolution, high-sensitivity upgraded Giant Metrewave Radio
Telescope observations of the Coma cluster (A1656) at 250-500 MHz and 550-850
MHz. At 250-500 MHz, 135 sources have extensions $>$ 0.45 arcmin (with
peak-to-local-noise ratio $> 4$). Of these, 24 sources are associated with
Coma-member galaxies. In addition, we supplement this sample of 24 galaxies
with 20 ram pressure stripped galaxies from Chen et al. (2020, eight are
included in the original extended radio source sample) and an additional five
are detected and extended. We present radio morphologies, radio spectra,
spectral index maps, and equipartition properties for these two samples. In
general, we find the equipartition properties lie within a narrow range (e.g.,
$P_{\rm min}$ = 1-3 dynes cm$^{-2}$). Only NGC 4874, one of the two brightest
central Coma cluster galaxies, has a central energy density and pressure about
five times higher and a radio source age about 50 % lower than that of the
other Coma galaxies. We find a diffuse tail of radio emission trailing the
dominant galaxy of the merging NGC 4839 group that coincides with the
"slingshot" tail, seen in X-rays. The southwestern radio relic, B1253$+$275,
has a large extent $\approx$ 32$^\prime$ $\times$ 10$^\prime$ ($\simeq$ 1.08
$\times$ 0.34 Mpc$^2$). For NGC 4789, whose long radio tails merge into the
relic and may be a source of its relativistic seed electrons, and we find a
transverse radio spectral gradient, a steepening from southwest to northeast
across the width of the radio source. Finally, radio morphologies of the
extended and RPS samples suggest that these galaxies are on their first infall
into Coma on (predominantly) radial orbits.
