The galaxy presents as a largely smooth, elliptical structure. The central region exhibits a bright, concentrated core, appearing yellowish in color, suggesting a population of older stars. The galaxy displays a gradual decrease in luminosity moving outward from the center, with a faint, diffuse halo surrounding the core. The overall shape is somewhat rounded but not perfectly spherical, showing a slight deviation towards a more intermediate form. There are no immediately apparent signs of spiral arms or significant dust lanes. No obvious signs of ongoing major merger events are observed, though there may be minor disturbances present given some asymmetry in the outer halo. The galaxy appears to be a relatively quiescent system with moderate mass and low levels of star formation.
