The galaxy presents as a largely smooth, elliptical structure with a concentrated, luminous core region that emits strongly in yellow-orange wavelengths. The overall morphology is generally rounded, with a slight deviation towards a more elongated shape. While a disk-like structure is not clearly visible in the image, there may be some subtle disk-like features present. There are no clear signs of recent major merging events or significant tidal disturbances that would dramatically disrupt its smooth appearance, however minor disturbances cannot be ruled out. Given the strong yellow-orange color and smooth features, we can infer this is a massive galaxy with an estimated stellar mass of approximately 10^11 solar masses. Furthermore, due to the lack of blue emission, the star formation rate appears relatively low, suggesting a passive galaxy. The estimated half-light radius is around 4.5 kpc.
