The galaxy appears as a centrally concentrated object, exhibiting a smooth, elliptical morphology. There is a noticeable radial color gradient, with a brighter, redder core transitioning to a bluer outer region. The galaxy's shape is generally round, with only a slight deviation towards a more elongated form. No prominent spiral arms or dust lanes are discernible. The overall appearance suggests a relatively evolved system with a significant population of older stars in the core, and ongoing, though likely subdued, star formation in the outer regions. There are no obvious signs of major mergers or significant tidal disturbances, though minor disturbances cannot be ruled out.
