The galaxy presents a largely smooth, elliptical morphology. There is a minimal presence of disk-like features. It exhibits a high degree of circularity, with a very slight deviation from being perfectly round, making it appear nearly spheroidal in shape. The light distribution appears relatively uniform across the galaxy, showing a concentrated central region that gradually fades outwards. A color gradient is present, with the core of the galaxy appearing more yellowish, gradually shifting to a redder hue at the periphery. No signs of ongoing merger events or major disturbances are observed. The galaxy's light profile suggests an evolved stellar population. The galaxy appears to be relatively massive and shows signs of a low star formation rate.
