The galaxy presents as a flattened, somewhat irregular shape when observed in these wavelengths. The central region exhibits a strong concentration of light, appearing nearly circular and very bright, suggesting a prominent galactic bulge or active galactic nucleus. A fainter, disk-like structure extends outward from this central region. 

The color distribution shows a general trend of bluer hues in the outer disk and a transition to redder hues closer to the galactic center. This could indicate ongoing star formation in the disk and an older stellar population in the core. There appear to be subtle asymmetrical features within the outer disk, suggesting possible disturbances or interactions. There is a slight indication of a tidal tail or disrupted arm on one side of the galaxy, which may be indicative of a minor merger.
