The galaxy presents as a relatively smooth, elliptical morphology. The core exhibits a high degree of central concentration, with a bright and luminous nucleus. The galaxy appears to be viewed at a moderate inclination, evidenced by its slightly elongated shape. There is a subtle color gradient, with the central regions appearing more yellow or white, possibly indicating an older stellar population compared to the outer regions, which exhibit hints of bluer hues. No distinct spiral arms are discernible, nor are there any obvious signs of a recent major merger event, although subtle asymmetries or distortions might be present, suggesting past gravitational interactions.
