The galaxy presents a generally smooth, elliptical morphology. It appears largely featureless, lacking prominent spiral arms or a distinct disk structure. The light distribution is concentrated towards the center, forming a bright, yellowish core. This core is surrounded by a more diffuse, less luminous halo that transitions into a blueish hue. There are hints of minor asymmetries or subtle extensions in the outer regions, though nothing that would suggest a major ongoing merger event. The overall color suggests a population of older stars dominating the stellar composition.
