The galaxy presents as a relatively smooth, elliptical or lenticular system. A concentrated central bulge dominates the morphology, exhibiting a yellowish-orange hue. The surrounding halo appears more diffuse, with a subtle greenish-blue tint, possibly indicating the presence of a population of younger, hotter stars or ionized gas. There are indications of some minor disturbances. The galaxy displays a generally rounded appearance, lacking strong indications of spiral arms or a distinct disk structure. 
