The galaxy presents a generally smooth morphology, appearing as a concentrated spheroid of light. There is evidence of a subtle disk-like structure, but it does not dominate the overall appearance. The galaxy appears relatively undisturbed, showing no obvious signs of a recent major merger event, although a minor disturbance cannot be ruled out. Color gradients within the galaxy show the core to be more yellow compared to the bluer outskirts of the spheroid, indicating a variance in the stellar population. The central region is the brightest part of the galaxy, gradually diminishing in luminosity towards the periphery.
