  We carry out deep near-ultraviolet (NUV) and far-ultraviolet (FUV) imaging of
an interacting galaxy system, comprised of a Seyfert type 1 galaxy NGC 7469 and
its companion IC 5283. Our aim is to resolve and map the star-forming regions
in the outer arms and look for signs of interaction between the two galaxies.
We used AstroSat Ultra Violet Imaging Telescope (UVIT) to obtain NUV and FUV
images of NGC 7469 in a range of filters. We have carried out photometry of
star-forming regions in the two galaxies and found their spatial distributions.
We also obtained the distributions of star formation rates (SFR) in NGC 7469
and IC 5283 using the estimates obtained from the FUV and NUV bands. We also
carried out Kolmogorov-Smirnov tests to look for differences in the SFRs in the
two galaxies. We derived the spectral energy distribution (SED), leading to the
determination of physical parameters, including the overall SFR, stellar mass
($\text{M}_{*}$), dust mass ($\text{M}_\text{Dust}$), and specific star
formation rates (sSFRs) in both the galaxies. Our NUV and FUV images show the
presence of an outer spiral arm that is better resolved. We have identified 33
new star-forming regions out of 51 total identified in the UVIT composite
image. Enhanced star formation activity is observed to coincide with the
interaction, and KS tests show that there are no significant differences in the
SFR distributions of NGC 7469 and IC 5283, indicating that the interaction
between the galaxies has not influenced their star formation processes
differently. The SED plots and the photometric results demonstrate that most of
the star formation activity is confined inside the central starburst (SB) ring.
