The galaxy presents as a smooth, elliptical morphology. It exhibits a concentrated central bulge, emitting primarily yellow-white light, suggesting a population of older stars. The galaxy displays a noticeable lack of defined spiral arms or dust lanes. There is a slight elongation present with a subtle gradient in color intensity outward from the core, transitioning to a dimmer, bluer halo. No obvious signs of active galactic nuclei or recent major merger events are apparent. The smooth, featureless appearance implies a relatively quiescent state with low levels of ongoing star formation.