The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a concentrated central bulge that transitions gradually into a more diffuse outer region. There is a slight elongation of the galaxy's shape. The color distribution indicates an older stellar population, with a yellow-red hue dominating, particularly within the core, suggesting evolved stars are prevalent. A faint blue tint is observed in the outer regions, which could indicate ongoing, but limited, star formation activity or a population of younger stars. No prominent spiral arms or significant dust lanes are visible. There are no major distortions or signs of an ongoing major merger event, though there could be minor disturbances. The galaxy's overall morphology points to a system that has largely settled into a stable configuration.
