The galaxy presents as a relatively compact, elliptical structure. Its morphology appears largely smooth, with a high degree of central concentration, showing a spheroid shape. The color distribution is predominantly uniform and reddish, suggestive of an older stellar population with little ongoing star formation. There is a lack of discernible spiral arms or disk-like features. The galaxy's roundness indicates it is more circular than elongated. No significant tidal features, major disturbances, or signs of an ongoing merger are detected.
