The galaxy presents a generally elliptical morphology, appearing largely smooth with a high degree of central concentration. There is an evident color gradient, transitioning from bluer hues in what appears to be the core region to more yellow-red tones in the outer areas. The structure is not perfectly symmetrical; there is a slight elongation. There is a hint of a possible minor disturbance, but the galaxy is generally well-defined and appears relatively undisturbed. The overall color profile suggests an intermediate population of stars with ongoing, albeit perhaps moderate, star formation.
