The galaxy presents an elliptical morphology, appearing largely smooth and featureless. Its overall color profile indicates a likely older stellar population, with a dominant yellowish-orange hue concentrated towards the galactic center. The outer regions exhibit a slight fading, suggesting a decreasing stellar density with increasing radial distance. There is a subtle hint of asymmetry, possibly indicative of a minor gravitational interaction or internal dynamic process, but without higher resolution imaging, this remains speculative. The galaxy does not display any prominent dust lanes or spiral arm structures. 
