The galaxy appears to be a relatively luminous, early-type system. Its morphology is generally smooth and elliptical, with a high degree of central concentration. The color profile suggests a population of older stars, appearing redder in color. There is no prominent disk structure or spiral arm features visible. Signs of recent or ongoing major merger activity are absent. There might be some minor disturbances, but the galaxy appears relatively relaxed and undisturbed. The estimated physical size is significant. It has a high stellar mass, with a very low specific star formation rate.
