The galaxy presents a largely smooth, elliptical morphology. A bright, concentrated central bulge dominates the structure, emitting a yellowish-white light that suggests an older stellar population. Surrounding the bulge is a more diffuse halo or envelope, displaying a faint bluish tint. This bluer color could indicate the presence of a younger, hotter stellar population, although the overall smoothness suggests that the light is not dominated by actively star-forming regions. The galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions. Its shape is generally round, lacking any prominent disk features or elongated structures. Overall, this galaxy seems to be a passively evolving, elliptical galaxy with a significant bulge component and a relatively smooth light distribution.
