The paper constructs a new family of Type IIB supergravity backgrounds that are dual to five-dimensional conformal field theories (CFTs) compactified and deformed by vacuum expectation values (VEVs) of certain operators. This generates an RG flow into a smooth background dual to non-supersymmetric gapped field theories in four dimensions. The authors study various holographic observables, including a monotonic quantity associated with the number of degrees of freedom, Wilson loops that interpolate between conformal and confining behavior with the possibility of screening, entanglement entropy, and holographic complexity. They also calculate the spectrum of spin-two glueballs in the field theories. The paper begins by introducing the general idea and the supergravity background, followed by a detailed analysis of the dual field theories and observables. The content is organized into sections covering the supergravity background, the dual field theories, and various holographic observables. The paper concludes with a discussion of the results and future directions for research.The paper constructs a new family of Type IIB supergravity backgrounds that are dual to five-dimensional conformal field theories (CFTs) compactified and deformed by vacuum expectation values (VEVs) of certain operators. This generates an RG flow into a smooth background dual to non-supersymmetric gapped field theories in four dimensions. The authors study various holographic observables, including a monotonic quantity associated with the number of degrees of freedom, Wilson loops that interpolate between conformal and confining behavior with the possibility of screening, entanglement entropy, and holographic complexity. They also calculate the spectrum of spin-two glueballs in the field theories. The paper begins by introducing the general idea and the supergravity background, followed by a detailed analysis of the dual field theories and observables. The content is organized into sections covering the supergravity background, the dual field theories, and various holographic observables. The paper concludes with a discussion of the results and future directions for research.