The galaxy presents as a centrally concentrated, smooth object with an elliptical morphology. Its core region is a bright, concentrated yellow hue that fades into a red halo. There is no visible evidence of spiral arms or a disk structure, nor signs of ongoing major mergers or tidal disturbances. The lack of distinct features suggests that the galaxy is primarily composed of an older stellar population, exhibiting limited current star formation activity. The light profile transitions smoothly from the central bulge outward, indicative of a well-relaxed system.
