The galaxy presents a largely smooth, elliptical morphology. Its light profile appears highly concentrated towards the center, with a gradual decrease in intensity outward. There is no discernible spiral arm structure or a distinct galactic disk. The overall color is on the redder end, suggesting an older stellar population with a lower rate of star formation. The galaxy's shape is more rounded than elongated. There is no obvious sign of a major ongoing merger or significant tidal disruption. There may be minor disturbances in the galaxy.
