The galaxy presents a flattened, disk-like structure when viewed from our observational perspective. It exhibits a somewhat smooth morphology, although with the limited resolution, subtle features may be present but not clearly discernible. The central region of the galaxy appears brighter, indicative of a higher concentration of stars and possibly a galactic bulge. There are some possible disturbances visible; one side appears to be warped and has a minor arm extending outwards. Overall, there appears to be a slight interaction or merger, but it is not well defined. 

The color distribution across the galaxy suggests variation in stellar populations. A reddish hue is apparent in the fainter areas, potentially signifying older, cooler stars, while some areas appear brighter and bluer. The difference in color would possibly indicate recent star formation occurring within that region. 
