The galaxy appears as a smooth, elliptical-shaped object with a bright, concentrated central bulge. The light distribution is relatively uniform across the main body, suggesting an older stellar population. There is a subtle color gradient, with the core appearing slightly yellower than the outer regions. This could indicate a higher concentration of older, redder stars in the center. No distinct spiral arms or dust lanes are discernible. The galaxy displays a high degree of axial symmetry, lacking any obvious signs of recent mergers or major disturbances. The overall morphology suggests a quiescent system with little ongoing star formation.
