The galaxy presents as an elliptical morphology, appearing largely smooth and spheroidal in structure with minimal discernible features such as spiral arms or a prominent disk. The light distribution is centrally concentrated with a gradual decline in intensity outward from the core. The color profile suggests an aging stellar population, indicated by the relatively red hue. There is no apparent ongoing major star formation, and it does not appear to be undergoing any major mergers or interactions with another galaxy. It is consistent with a quiescent galaxy that has largely exhausted its supply of gas for forming new stars.