The galaxy presents as an elliptical morphology, appearing largely smooth and rounded in shape. There is a slight color gradient from the center outwards, hinting at potential variations in stellar populations or dust distribution. The galaxy exhibits a relatively concentrated light profile, suggesting an older stellar population. No apparent spiral arm structures or significant dust lanes are visible. The galaxy appears relatively isolated, with no obvious signs of ongoing major mergers or tidal disturbances. The color suggests a passively evolving galaxy with low recent star formation.
