The galaxy appears to be a relatively smooth, elliptical galaxy. The central region exhibits a bright, concentrated light, suggesting a high stellar density or possible active galactic nucleus. The overall color is yellowish-orange, indicative of an older stellar population dominated by redder stars with only a hint of young blue stars. The galaxy appears largely undisturbed, with no obvious signs of recent mergers or tidal interactions with other galaxies. The galaxy is well-resolved. There are no prominent spiral arms or a well-defined disk. Its overall shape is roughly circular, appearing nearly face-on. The galaxy's halo is faint and diffuse, exhibiting a gradual decrease in luminosity from the core towards the outer edges. There seems to be an absence of significant dust lanes or patches within the galaxy. The smooth light distribution and color suggest that it is a passively evolving galaxy with a relatively low rate of star formation.
