The galaxy presents as a relatively smooth, centrally concentrated object with a high degree of circular symmetry. There is a noticeable color gradient, transitioning from a yellowish-white hue in the core to a slightly redder color in the outer regions. No distinct spiral arm structures or prominent dust lanes are discernible. The overall morphology is consistent with an elliptical galaxy or a lenticular galaxy seen at a low inclination angle. There's no obvious sign of major merging activity or significant tidal disturbance. The faint redder outer regions suggest a population of older, cooler stars, while the brighter, yellower core indicates a region with either younger stars or a greater density of stars overall.
