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TCP J18224935-2408280 was reported to be in outburst on 2021 May 19.Follow-up spectroscopic observations confirmed that the system was a symbioticstar. We present optical spectra obtained from the Himalayan Chandra Telescopeduring 2021-22. The early spectra were dominated by Balmer lines, He I linesand high ionization lines such as He II. In the later observations, Ramanscattered O VI was also identified. Outburst in the system started as a discinstability, and later the signature of enhanced shell burning and expansion ofphotospheric radius of the white dwarf was identified. Hence we suggest thisoutburst is of combination nova type. The post-outburst temperature of the hotcomponent remains above 1.5 x 10$^5$ K indicating a stable shell burning in thesystem for a prolonged time after the outburst. Based on our analysis ofarchival multiband photometric data, we find that the system contains a coolgiant of M1-2 III spectral type with a temperature of $\sim$ 3600K and a radiusof $\sim$ 69 R$_\odot$. The pre- and post-outburst light curve shows aperiodicity of 631.25 $\pm$ 2.93 d; we consider this as the orbital period.

TCP J18224935-2408280: a symbiotic star identified during outburst