The galaxy presents an overall elliptical morphology, appearing largely smooth and lacking prominent spiral arm structures. The central region exhibits a high degree of concentration, with a bright, almost stellar-like nucleus suggesting a significant concentration of stars or possibly an active galactic nucleus. The galaxy's light profile appears relatively uniform, with a gradual decrease in intensity from the center outwards, and it has a slight disclike shape. There may be some minor disturbances in the symmetry of the galaxy, but no major ongoing merger events are apparent in this image.
