The observed galaxy presents a disk-like morphology, although the relatively small angular size complicates detailed analysis. The central region displays a bright, concentrated luminosity, suggesting a prominent galactic nucleus. Surrounding the core, a flattened structure is visible, indicative of a disk component. The color gradient suggests that the outer regions of the disk may contain a younger population of stars than the nuclear area. While a spiral arm structure is not immediately apparent, there is the possibility of faint, loosely wound arms or flocculent structure within the disk; further analysis might require image enhancement or more precise photometric data. There appears to be some disturbance to the disk, which might be due to a small degree of tidal interaction with a smaller galaxy.
