The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape appears elliptical, with a high degree of symmetry about the central region. The color gradient suggests a fairly evolved stellar population, with the central bulge exhibiting a yellowish-orange hue indicative of older, redder stars. A subtle greenish-blue halo surrounds the bulge, suggesting the presence of a younger, bluer stellar population, or possibly ongoing, low-level star formation in the outer regions. No prominent spiral arms or distinct features are discernible, suggesting it could be an elliptical galaxy or a lenticular galaxy with a weak disk. The absence of strong dust lanes or tidal features suggests that this galaxy has not undergone a recent major merger. Overall, it appears to be a galaxy with a significant spheroidal component and likely a large stellar mass.
