The galaxy presents as a largely smooth, elliptical form. A discernible central bulge exhibits a concentrated luminosity, with colors trending towards the red end of the spectrum. Moving outward from the core, the light distribution becomes more diffuse. A slight blue-ish tint surrounds the central region, possibly indicating the presence of some younger stellar populations or ongoing star formation, though limited. There is minimal evidence of spiral arm structure or significant dust lanes within the observable light. The overall shape is generally rounded but appears slightly elongated along one axis, presenting a more elliptical appearance than circular. No major merger events or tidal disturbances are immediately apparent, though a hint of minor irregularity exists in the outer halo.
