The galaxy presents as a relatively smooth, centrally concentrated object. It appears elliptical or lenticular in form, exhibiting high degree of roundness, lacking any obvious spiral arms or bar structures. The core exhibits a bright, yellowish-white hue, indicative of an older stellar population. The outer regions display a fainter, more diffuse halo with a slightly reddish tint. The structure implies a galaxy that has largely ceased active star formation. No prominent dust lanes or other features indicative of significant gas content are visible. There are no signs of tidal disturbances or interactions with other galaxies in this image. The overall morphology suggests a galaxy that has undergone significant internal dynamical relaxation.
