The galaxy presents as a relatively smooth, elliptical-like structure with a bright, concentrated central bulge. The core exhibits a yellowish-white hue, suggesting an older stellar population. Moving outwards from the core, the color gradually transitions to a bluish-white, hinting at the presence of younger stars in the outer regions. No distinct spiral arm structures are discernible. There is a subtle asymmetry in the outer halo, and no signs of any major ongoing merger events, although there is possibly a minor tidal disturbance. The overall morphology indicates it is likely a mature galaxy.
