This galaxy appears to be a relatively smooth, elliptical system. It exhibits a central bulge that is significantly brighter and more concentrated than the surrounding halo. The light distribution suggests that it is largely composed of older stellar populations, giving it a yellowish hue, particularly in the core. There is a slight elongation to the galaxy's shape, leaning towards an intermediate apparent ellipticity. No prominent spiral arms or significant dust lanes are visible. There might be faint disturbances in the outer halo, but it mainly appears undisturbed. The galaxy shows moderate star formation activity. Overall, it seems to be an elliptical galaxy with a substantial mass and size.
