This galaxy presents a largely smooth, elliptical morphology. Its overall shape appears moderately rounded. The galaxy exhibits a concentration of light toward the center, suggesting a prominent galactic nucleus. The color profile indicates a presence of older stellar populations, potentially dominated by redder stars, with some evidence of younger, bluer stars throughout the galaxy. While the galaxy is mostly uniform in appearance, there is a slight indication of possible minor disturbances. These could be from past interactions, but more data would be needed to confirm this. No distinct spiral arms or a well-defined disk structure is observed, supporting its classification as an elliptical galaxy.
