The galaxy presents as a moderately bright, elliptical structure with a smooth, featureless morphology. The light profile suggests a concentration of older stellar populations toward the center, exhibiting a yellowish-gold hue that diminishes toward the outer regions. There is an indication of a slight disc-like structure but it is a mostly spheroidal galaxy. The outer regions display a faint bluish tint, potentially indicative of ongoing, but likely weak, star formation within the galaxy's outskirts. The galaxy appears relatively undisturbed, lacking any obvious signs of tidal interactions or recent mergers and no dust lanes are visible.
