The galaxy presents as a largely featureless elliptical or lenticular structure. The central region exhibits a high surface brightness, suggesting a dense concentration of stars. The light profile appears smooth and gradually fades towards the outer edges of the galaxy, lacking prominent spiral arms or distinct features like dust lanes. There is little to no apparent substructure, and the overall morphology suggests a relatively evolved system. The color profile indicates a predominantly older stellar population, as evidenced by the reddish-yellow hue, although there may be a small component of recent star formation. No signs of any on-going or recent major merger events are visible.
