The observed galaxy presents a disk-like morphology, viewed at an oblique angle, with the disk noticeably tilted relative to our line of sight. Prominent spiral arm structures are evident, exhibiting a somewhat flocculent nature. These arms appear well-defined, originating from the central region and extending outwards. The galactic bulge appears moderately sized. Color gradients suggest ongoing star formation within the spiral arms, evidenced by the presence of bluer regions. There is an indication of a possible weak bar structure. The galaxy does not appear to be undergoing any major interactions or significant mergers, although subtle disturbances may be present.
