The galaxy presents as a largely smooth, elliptical-like structure. It exhibits a high degree of central concentration, with a bright, diffuse core. There is a distinct color gradient visible, transitioning from a yellowish-white at the center to a redder hue in the outer regions. No prominent spiral arms, bars, or other distinct features are readily apparent, suggesting a relatively relaxed morphology. Close inspection reveals a slight deviation from perfect circularity, hinting at the possibility of minor tidal interactions or internal disturbances. The overall impression is that of a massive, evolved system with a diminished rate of active star formation.
