The galaxy presents as a relatively smooth, elliptical structure. The core region exhibits a concentrated, bright, yellowish-orange hue, suggesting an older stellar population and potentially a significant population of dust. Moving outward from the core, a gradual decrease in surface brightness is observed, with the color shifting towards a slightly greener tinge. This suggests the possibility of some ongoing, albeit low, levels of star formation in the outer regions, or perhaps a different population of stars. The overall shape is generally round. No significant tidal features or major disturbances are apparent. There are no visible spiral arm structures. The galaxy exhibits a moderate redshift, indicating that the light has been stretched due to the expansion of the universe as it traveled to us.
