The galaxy presents as a largely elliptical structure, with a high degree of central concentration indicated by a bright, almost stellar-like core. The light profile appears relatively smooth, with no prominent spiral arms or distinct features discernible. The isophotes are generally round, showing only minor deviations from perfect circularity. Faint extensions suggest the possibility of a diffuse halo surrounding the main body of the galaxy. Color gradients indicate the core is more red than its surrounds, with bluer colors visible at the periphery. There is no obvious indication of ongoing major merger activity.
