The galaxy presents a flattened, disk-like morphology, observed at a moderate inclination to our line of sight. The central region exhibits a brighter, more concentrated luminosity profile, suggesting the presence of a galactic bulge. Evident within the galaxy are regions of enhanced blue emission. This is suggestive of ongoing star formation activity, which is often associated with younger, hotter stellar populations. The outer regions of the galaxy appear fainter and less structured. There may be some minor tidal disturbances or asymmetries detectable in its morphology. Overall, the galaxy appears to be a disk galaxy with some evidence of internal activity and potential minor interactions.
