The galaxy presents an elliptical morphology, with a smooth light distribution that suggests an older stellar population. The core appears bright and concentrated, possibly indicating a supermassive black hole at its center. There is a subtle disklike asymmetry about the minor axis suggesting a possible recent merger event. The galaxy is a moderate distance, allowing details in the arms to not be observed. The overall color indicates a low star formation rate, likely due to the galaxy's aging stellar population.
