The galaxy appears as a roughly elliptical, well-defined entity. The light profile suggests a high degree of central concentration with a smooth, gradual falloff in luminosity towards the outer regions. The primary color is yellow-white, indicative of an older stellar population, with a slight color gradient towards the center becoming more yellow. There is no apparent dust lane or significant substructure present. The overall morphology is relatively undisturbed, with no signs of ongoing major mergers. It appears as a highly rounded system.
