The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The core exhibits a bright, yellowish-white hue, potentially indicating an older stellar population. Extending outward from the core, the galaxy displays a gradual decrease in luminosity. The outer regions exhibit a bluer color profile, possibly suggesting the presence of younger stars and ongoing star formation, although at a low rate. There is no prominent disk structure visible, nor are there any signs of major morphological disturbances or ongoing mergers. The overall appearance suggests a relatively evolved system transitioning towards a more passive state.