The galaxy presents a largely smooth, elliptical morphology. Its central bulge is a bright, concentrated region exhibiting a yellow-orange hue, indicative of an older stellar population. The radial light profile suggests a gradual decrease in luminosity from the core outwards. Faint, diffuse, bluish-greenish outer regions are visible, indicating the possibility of some younger stars or ongoing, but minimal, star formation activity at the galaxy's periphery. No distinct spiral arms or bar features are readily apparent, although the image resolution is a limiting factor. The overall symmetrical, rounded shape points to a system that has undergone significant dynamical relaxation. There is no evidence of any major merger events or significant tidal disturbances in the immediate vicinity.
