The galaxy presents a primarily smooth morphology, with an overall elliptical shape. Its central region exhibits a high degree of luminosity, suggesting a significant concentration of stars within the galactic nucleus. The color gradient transitions from a yellowish-white core to a reddish-orange hue in the outer regions, indicating a potential variation in stellar populations, with older, redder stars dominating the periphery. There is a very slight hint of a disk-like structure, although it is very subtle. No distinct spiral arms or other prominent features are readily apparent. There are no other galaxies nearby that appear to be in the process of merging with this particular galaxy. The relative lack of blue light suggests moderate star formation activity.
