The galaxy presents as a relatively smooth, elliptical-like structure. Its color profile suggests a population of older stars, with a dominant yellowish-orange hue. There is no apparent spiral arm structure or significant dust lane obscuration. The galaxy appears largely undisturbed, lacking any obvious signs of recent major merger activity or tidal distortions in its overall shape, though some minor asymmetry cannot be ruled out. The object's smooth morphology suggests a classification leaning towards an early-type galaxy. The light is concentrated towards the center and fades away smoothly towards the outer edges.

