The galaxy presents a largely smooth, elliptical morphology. The central region exhibits a concentrated, bright core, with a gradual decrease in luminosity towards the outer edges. The color gradient transitions from a warmer, yellowish-white center to slightly cooler, greenish-yellow hues in the surrounding halo. No distinct spiral arms or bar structures are discernible. There is no evidence of major tidal disturbances or ongoing merger events. A slight asymmetry can be observed, though the galaxy appears predominantly rounded in shape. The overall appearance suggests an evolved stellar population, likely dominated by older stars. The galaxy exhibits relatively low levels of star formation.
