The galaxy presents as a centrally concentrated object with a largely smooth morphology. It appears elliptical or spheroidal in shape, exhibiting a high degree of radial symmetry. The core region shows a bright, concentrated luminosity, suggesting a dense population of stars. The overall color is predominantly yellow, indicating a stellar population that is relatively old. No obvious spiral arms or dust lanes are visible, supporting the classification as an elliptical galaxy. There are no signs of ongoing major mergers or tidal distortions in its apparent structure, though subtle disturbances cannot be entirely ruled out.
