The galaxy presents as a centrally concentrated object, exhibiting a smooth, elliptical morphology. It displays a gradual decrease in brightness from its core outwards, lacking any sharply defined spiral arms or a prominent disk structure. The galaxy appears to be in an intermediate stage of roundness, being neither perfectly spherical nor significantly elongated. There is no evidence of major ongoing mergers or significant tidal disturbances.

The galaxy exhibits a color profile indicative of a population of aging stars. The core appears yellowish-white, suggesting the presence of evolved stars, while the outer regions are a bit more reddish. Overall, the colors show little current star formation activity.
