The galaxy presents a relatively smooth, elliptical morphology. It exhibits a generally flattened, but not highly elongated, shape. The light distribution appears concentrated towards the center, with a gradual decrease in luminosity moving outwards. There's a hint of blueish hue emanating from its center, suggesting the presence of younger stars or an active galactic nucleus. The overall structure doesn't show any signs of major disturbances or ongoing mergers, but slight asymmetries may be present. Overall, the galaxy appears to be a relatively quiescent system.
