The galaxy presents as a relatively smooth, elliptical form with a high degree of central concentration. A prominent, bright core region is visible, exhibiting a yellow-orange hue, suggestive of an older stellar population. The outer regions of the galaxy display a fainter, more diffuse appearance, transitioning to a bluish color. This color gradient may indicate some ongoing star formation within the galaxy, primarily occurring in its outer reaches. The overall shape is elongated, but not extremely so, possibly indicating a transitional form between a perfectly spherical and a flattened elliptical galaxy. The system shows no obvious signs of major mergers or significant tidal disturbances, although there is a subtle suggestion of asymmetry in the outer halo, implying the possibility of a minor interaction in its past.
