The galaxy presents as a primarily smooth, elliptical structure, exhibiting a high degree of central concentration with a nearly circular morphology. There is a slight deviation from perfect circularity, though no prominent disk-like features are observed. The galaxy's color suggests an older stellar population, with a relatively low rate of star formation. No significant signs of recent or ongoing merger activity are apparent, although there is an extremely small hint of minor disturbance present. The overall appearance indicates a relatively evolved system.
