The galaxy presents a flattened, disk-like morphology, exhibiting a complex structure within the disk itself. The central region appears bright, possibly indicating a concentration of stars or an active galactic nucleus. Around the central region, there appears to be a surrounding area that is less bright than the central nucleus, but significantly brighter than the outer disk. It shows a mottled or clumpy texture, suggesting varying densities of stellar populations, gas, and dust. Distinct features like spiral arms or a bar structure are not clearly discernible in this image, though the disk appears slightly asymmetric, possibly due to tidal interactions or internal dynamics. There may be a merging event occurring, as small irregularities in the shape could indicate disturbance of some kind. Color variations within the disk suggest differences in stellar populations, with bluer regions potentially indicating younger, hotter stars and star formation. The galaxy shows moderate elongation. Overall, the galaxy exhibits signs of ongoing activity or recent interactions affecting its morphology and stellar distribution.
