This galaxy presents an elliptical morphology, appearing largely smooth and centrally concentrated with a notable lack of distinct spiral arm structure. The light profile suggests a relatively evolved stellar population, indicated by a yellowish-white hue toward the core, transitioning to a bluer color in the outer regions. There may be some minor disturbances, but overall the galaxy exhibits a settled structure, without indications of a recent major merger event. Its roundness is somewhere in between a circle and a more elongated, cigar shape. The mass estimate appears high suggesting that the galaxy is a very massive galaxy. The central region exhibits high luminosity, suggesting a high concentration of stars or possibly the presence of an active galactic nucleus. The rate of new stars being formed is relatively low.
