The galaxy presents a generally smooth morphology. The object appears as an elliptical galaxy, lacking any strong spiral arm structures or a well-defined disk. The light distribution indicates a concentration towards the center, with a gradual decrease in surface brightness moving outwards. It shows a slightly elongated shape, appearing somewhat flattened rather than perfectly spherical. There is a subtle hint of disturbance in the outer regions of the galaxy, indicating a potential minor interaction or past merger event. The core region exhibits a yellow to golden hue, suggesting an older stellar population, while the outer regions appear bluer.
