The galaxy presents a generally smooth, elliptical morphology. A bright, concentrated nucleus is evident, indicative of a substantial central mass concentration. The color profile appears relatively uniform, exhibiting a slight bluish tint. The outer regions show a gradual decrease in surface brightness, blending smoothly into the background sky. There may be some evidence of subtle disturbances or minor features in the outer halo region of the galaxy, but these are not distinctly defined. The overall structure suggests a relatively evolved system, with a moderate stellar mass and a suppressed star formation rate. It presents a generally rounded appearance.
