The galaxy presents as a single, largely featureless entity. The object is centrally concentrated with a smooth, elliptical light distribution. The core region exhibits a yellowish-white hue, indicating a probable population of older stars. There is a decrease in luminosity as one moves radially outward from the core, fading into a faint reddish halo surrounding the galaxy. No spiral arms or dust lanes are discernible within this limited resolution. Overall, the morphology suggests a spheroidal galaxy, likely an elliptical galaxy with a high degree of central concentration.
