The galaxy presents a relatively smooth, elliptical morphology. Its light is dominated by a central bulge, displaying a yellowish hue which suggests a population of older stars. There is little evidence of significant spiral arm structure or dust lanes within the optical wavelengths observed. The galaxy appears largely undisturbed, with no major signs of ongoing mergers or tidal distortions. The outer regions fade gradually into the background, exhibiting a subtle gradient in color suggesting varying stellar populations and metallicities within the galaxy's halo. Overall, the galaxy exhibits properties consistent with a mature, quiescent system.
