The galaxy presents as a relatively smooth, elliptical morphology. Its color profile suggests an older stellar population. The light is concentrated towards the center with only a slight color difference from the center to the outer edges of the galaxy. There are no discernible spiral arms or distinct features indicative of active star formation, though the slight bluish tinge suggests some is occurring. Overall, the galaxy exhibits a largely spheroidal shape with an even distribution of light, indicating a system that has undergone substantial dynamical relaxation.
