The galaxy appears to be a single, relatively symmetrical object, likely an elliptical galaxy. It exhibits a smooth, concentrated central bulge. The light distribution suggests a high degree of radial symmetry, with a gradual decrease in luminosity from the center outwards. The galaxy displays a yellowish-white hue in its core, hinting at an older stellar population dominating the central region. Fainter, more diffuse light extends outwards from the core, forming a surrounding halo. There is little evidence of spiral arms or significant dust lanes and star formation, supporting a classification as an elliptical galaxy. There is no apparent sign of major mergers or significant disturbances in the galaxy's structure.
