The galaxy presents an elliptical morphology, exhibiting a smooth, diffuse light distribution with no readily apparent spiral arm structure. The central region displays a concentrated luminosity, appearing a yellow-orange hue, suggesting a population of older stars. Moving outwards from the core, the galaxy fades into a more diffuse, bluish halo. The shape appears mostly regular, without noticeable tidal distortions or signs of ongoing major mergers. Subtle color variations might indicate regions of differing stellar populations or dust content within the galaxy's structure. The overall appearance indicates a relatively evolved system, likely a lenticular or elliptical galaxy.
