This galaxy presents as a relatively smooth, elliptical-type morphology. It appears largely spheroidal in shape with minimal discernible substructure or features. The galaxy exhibits a color gradient, with the central region appearing more yellowish, suggesting an older stellar population, and a slight shift towards redder hues in the outer regions. The galaxy does not show any obvious signs of active star formation regions or significant dust lanes, indicating that its star formation rate is low. Based on its red shift, its light has been stretched as it travels to earth, as it recedes away from us.
