The galaxy presents as a centrally concentrated, luminous object, with a smooth and largely featureless appearance. Its overall shape is elliptical, exhibiting a high degree of circularity. There are no readily discernible spiral arms or a prominent disk structure. The color profile suggests an older stellar population, with a yellow-orange hue dominating the central regions, and a slight bluer tinge in the surrounding halo. The smooth morphology indicates a likely lack of major ongoing star formation, and the dominance of evolved stars. There are no signs of significant tidal disturbances or ongoing mergers, though the possibility of a minor interaction cannot be completely ruled out due to some possible distortion. 
