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We present the first X-ray dedicated study of the galaxy cluster A795 and ofthe Fanaroff-Riley Type 0 hosted in its brightest cluster galaxy. Using anarchival 30 ks \textit{Chandra} observation we study the dynamical state andcooling properties of the intracluster medium, and we investigate whether thegrowth of the radio galaxy is prevented by the surrounding environment. Wediscover that A795 is a weakly cool core cluster, with an observed massdeposition rate $\lessapprox 14\,$ M$_{\odot}$yr$^{-1}$ in the cooling region(central $\sim$66 kpc). In the inner $\sim$ 30 kpc we identify two putativeX-ray cavities, and we unveil the presence of two prominent cold fronts at$\sim$60 kpc and $\sim$178 kpc from the center, located along a cold ICM spiralfeature. The central galaxy, which is offset by 17.7 kpc from the X-ray peak,is surrounded by a multi-temperature gas with an average density of$n_{\text{e}} = 2.14 \times 10^{-2}$ cm$^{-3}$. We find extended radio emissionat 74-227 MHz centered on the cluster, exceeding the expected flux from theradio galaxy extrapolated at low frequency. We propose that sloshing isresponsible for the spiral morphology of the gas and the formation of the coldfronts, and that the environment alone cannot explain the compactness of theradio galaxy. We argue that the power of the two cavities and the sloshingkinetic energy can reduce and offset cooling. Considering the spectral andmorphological properties of the extended radio emission, we classify it as acandidate radio mini-halo.

A Chandra study of Abell 795 -- a sloshing cluster with a FR0 radio galaxy at its center