The galaxy presents as an elliptical morphology, with a smooth, featureless appearance. There is a high degree of central concentration, as evidenced by the bright, yellowish core that gradually fades towards the outer edges. The galaxy's shape deviates slightly from being perfectly circular, exhibiting a mild elongation along its major axis. There is no discernible spiral arm structure or evidence of active star formation regions within the visible light spectrum. The overall color suggests a population of older stars, with minimal amounts of dust obscuration. The galaxy's structure appears relatively undisturbed, indicating no recent major merger events.
