  We present here the information on the design and performance of the recently
commissioned 2.5-meter telescope at the PRL Mount Abu Observatory, located at
Gurushikhar, Mount Abu, India. The telescope has been successfully installed at
the site, and the Site Acceptance Test (SAT) was completed in October 2022. It
is a highly advanced telescope in India, featuring the
Ritchey-Chr$\acute{e}$tien optical configuration with primary mirror active
optics, tip-tilt on side-port, and wave front correction sensors. Along with
the telescope, its two first light instruments {namely Faint Object Camera
(FOC) and PARAS-2} were also integrated and attached with it in the June 2022.
{FOC is a} camera that uses a 4096 X 4112 pixels detector SDSS type filters
with enhanced transmission and known as u', g', r', i', z'. It has a limiting
magnitude of 21 mag in 10 minutes exposure in the r'-band. The other first
light instrument PARAS-2 is a state-of-the-art high-resolution fiber-fed
spectrograph operates in 380-690 nm wave-band, aimed to unveil the super-Earth
like worlds. The spectrograph works at a resolution of $\sim$107,000, making it
the highest-resolution spectrograph in Asia to date, which is under
{ultra}-stable temperature and pressure environment, at 22.5 $\pm$ 0.001
$^{\circ}$C and 0.005 $\pm$ 0.0005 mbar, respectively. Initial calibration
tests of the spectrograph using a Uranium Argon Hollow Cathode Lamp (UAr HCL)
have yielded intrinsic instrumental RV stability down to 30 cm s$^{-1}$.
