The galaxy appears to be elliptical in shape, exhibiting a smooth, centrally concentrated light profile. The core of the galaxy shows a yellow-white color, indicating an older stellar population. The outer regions of the galaxy become increasingly redder, suggesting a gradient in stellar age or metallicity, with older or more metal-rich stars residing further from the center. There is no obvious presence of spiral arms or dust lanes. The galaxy appears relatively undisturbed, without significant tidal features or signs of recent merger activity.
