The galaxy presents a smooth, elliptical morphology with a high degree of roundness. There appears to be a centrally located nucleus, which is likely its supermassive black hole. The galaxy exhibits a blue hue, suggestive of some young stars. There is no apparent spiral arm structure, bar, or other prominent features typically associated with disk galaxies. No significant tidal disturbances or merger features are detected, suggesting that the galaxy has had a relatively stable evolutionary history.
