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Fig. 3.

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GALFIT decomposition of NGC 6902A and UVIT J2022. Panel a: model obtained from the fitting of NGC 6902A and UVIT J2022 with the 3+2 Sersic component in the r band. Panel b: model image of UVIT J2022. The size scale is the same in panels a and b. However, the grayscale in panel b is different to show the extent of UVIT J2022. Panel c: total model average surface brightness profile of UVIT J2022 in the r band, obtained from GALFIT (solid curve). The dotted and dashed curves show the Sersic profiles for the inner central bar-like structure and disk component, respectively. Panel d: surface density of UVIT J2022.

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