The galaxy presents as a relatively smooth, elliptical-like structure. A bright, concentrated core region is visible, suggesting a high stellar density. Moving outwards from the core, a more diffuse halo is observed, exhibiting a subtle color gradient from yellowish-white near the center to a slightly bluer hue in the outer regions. There is no apparent spiral arm structure or significant dust lane obscuration. The overall light distribution appears even and symmetrical, with no obvious signs of major tidal disturbances or ongoing merger activity. Minor asymmetrical features cannot be ruled out due to the image resolution. The galaxy exhibits a degree of roundness, appearing neither perfectly spherical nor highly elongated.
