The galaxy presents as a predominantly smooth, elliptical morphology. It is characterized by a central, concentrated bulge exhibiting a yellowish-orange hue, suggesting a population of older, cooler stars. The color gradient transitions subtly towards the outer regions, displaying a slight greenish tint. This could indicate regions of limited, ongoing star formation, although the overall color profile suggests a relatively quiescent galaxy. The galaxy appears to be largely undisturbed, showing no obvious signs of tidal interactions or major mergers. Its overall structure is well-defined and regular, indicative of a dynamically relaxed system.
