The galaxy exhibits a primarily smooth morphology. It presents a bright central region, which suggests a significant concentration of stars or an active galactic nucleus. Surrounding this core is a fainter, more diffuse halo. There is possible evidence of minor tidal disturbances, potentially indicating an interaction or merger event. The galaxy exhibits a somewhat distorted structure, with hints of asymmetrical features. The color profile suggests a mix of stellar populations, with some regions appearing bluer, indicating younger, hotter stars, while others are redder, indicative of older, cooler stars. There is a hint of a disk.
