The galaxy presents as a relatively smooth, elliptical-shaped structure. It exhibits a dominant central bulge with a high degree of circularity. There is very little indication of spiral arm features or disk-like morphology. The color profile suggests a population of older stars, with a yellowish-orange hue indicative of lower recent star formation activity. No major disturbances, tidal tails, or evidence of an ongoing major merger event are apparent. Minor asymmetry or subtle disturbances can not be ruled out at this resolution. The overall impression is that of a quiescent galaxy.
