The galaxy presents as a moderately luminous elliptical type, with a smooth, diffuse appearance. It exhibits an intermediate ellipticity, appearing somewhat flattened but not highly elongated. The color profile suggests a dominant population of older stars, indicated by the reddish-orange hue concentrated toward the core. A subtle gradient is observed towards the outer regions, with a faint bluish-greenish halo. There is no discernible spiral structure or distinct dust lane features. Minor distortions are present. These features point towards a relatively quiescent galaxy with a low rate of ongoing star formation.
