This galaxy exhibits an elliptical morphology, appearing largely smooth with a slight elongation. The central region presents a high concentration of light, indicating a prominent galactic nucleus. The color profile suggests a relatively older stellar population, with a yellowish-orange hue dominating the central and inner regions, transitioning to slightly redder tones in the outer halo. There are no apparent spiral arms or distinct dust lanes. The general appearance indicates a galaxy that has likely undergone significant evolution, with lower rates of current star formation. There are no signs of any major merging events, however some minor disturbances cannot be ruled out.
