The galaxy appears as a relatively compact, elliptical-like system. Its overall color profile suggests a population of older stars, with a yellowish-red hue dominating the central region. There is a lack of any prominent spiral arm structures or dust lanes. The light distribution appears smooth and concentrated, indicating a high degree of radial symmetry. While there appears to be a bright central core, there is also a gradual fade to its outer regions, making it appear hazy. The morphology is most likely that of an elliptical galaxy with little or no ongoing major star formation.
