This galaxy exhibits an irregular morphology. The primary body of the galaxy appears diffuse, with a notable concentration of luminosity toward the center. There is a secondary concentration of luminosity to one side of the main body, suggesting a possible tidal interaction or ongoing merger. The color gradient indicates a higher concentration of older stellar populations toward the core, with relatively bluer regions extending outwards, potentially indicative of more recent star formation activity in the outer regions. No distinct spiral arm structures are visible. Overall, the galaxy presents a disturbed and dynamically active appearance.
