The galaxy presents a largely smooth morphology. It appears elliptical, with a high degree of central concentration, and a gradual decrease in luminosity moving outward. The galaxy exhibits a near-perfect roundness. No distinct features such as spiral arms, bars, or dust lanes are discernible. There is no obvious sign of ongoing merger activity or tidal disturbance. The galaxy’s color is generally yellowish-white, indicative of an older stellar population. The estimated size is relatively compact.
