The galaxy presents a generally smooth and elliptical morphology. Its core exhibits a bright, concentrated luminosity, suggestive of a significant stellar population and potentially a supermassive black hole at its center. The galaxy appears relatively undisturbed, with no visible signs of recent major mergers or tidal interactions. The color profile indicates a higher concentration of older stellar populations, particularly in the central regions, which display a yellowish hue. The outer regions show some bluer colors, suggesting the presence of younger stars or ongoing star formation, albeit at a low rate. The overall structure suggests a well-evolved galaxy with a substantial spheroidal component.
