The galaxy presents as a luminous, elliptical-shaped structure. Its core exhibits a concentrated intensity, suggesting a high density of stars and possibly a supermassive black hole at its center. The luminosity appears to gradually decrease from the core outwards, forming a smooth halo. The galaxy shows a lack of defined spiral arms or significant dust lanes within the image, contributing to its smooth appearance. There is a slight elongation along one axis, suggesting a mild flattening. The overall color appears yellow, indicating a predominantly older stellar population with a low star formation rate. The morphological characteristics are indicative of a galaxy undergoing a stage where star formation has subsided.