The galaxy presents as a generally smooth object, with an elliptical morphology dominating its overall shape. A highly concentrated, bright central bulge is observed, exhibiting a yellowish-white hue, suggesting an older stellar population. Progressing outwards from the core, the galaxy transitions into a more diffuse halo with a subtle bluish tint, hinting at the presence of younger, hotter stars in its outer regions, potentially indicating ongoing or recent star formation. There is no discernible spiral arm structure or prominent dust lanes. Faint asymmetric features exist, likely due to minor gravitational interactions. The overall appearance suggests an evolved system, possibly an elliptical galaxy nearing the end of its star-forming period.
