The galaxy presents a predominantly smooth, elliptical morphology. Its light profile appears concentrated towards the center, indicating a dense galactic nucleus. The color gradient transitions from a yellow-white core to a redder, fainter periphery. There is a subtle suggestion of a disk component, yet the overall structure lacks the well-defined spiral arms typically associated with disk galaxies. Minor disturbances may be present in its structure, likely indicating that it could be undergoing a minor merging event.