The galaxy presents a largely smooth, elliptical morphology. The central region is characterized by a bright, concentrated core, suggesting a high stellar density and potentially hosting a supermassive black hole. There is a gradual decrease in luminosity moving outwards from the center, with no apparent spiral arm structure or significant dust lanes visible. The galaxy appears relatively undisturbed, with no clear signs of recent major mergers or tidal interactions. Faint, diffuse light extends outward from the main body, forming a halo of older stars. The overall color index suggests a population dominated by older, redder stars, indicative of a lower ongoing star formation rate. The galaxy appears mostly round, with minimal distortion from its central core. There are no visible signs of active galactic nuclei activity, such as prominent jets or ionized gas emission.
