The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. The core exhibits a bright, yellowish-white hue, indicative of a population of older stars. Progressing outwards from the core, the light gradually decreases in intensity, transitioning to a more diffuse, yellowish-orange halo. There is little evidence of distinct spiral arms or prominent dust lanes. The overall structure suggests a relatively evolved galaxy, potentially an elliptical or lenticular type, viewed face-on or at a slight inclination. There is a subtle hint of a possible tidal feature or minor asymmetry.
