The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge with a gradual decrease in luminosity outward. There is little evidence of distinct spiral arm structures or significant dust lanes within the galaxy. The overall color appears slightly redder, suggesting an older stellar population. The galaxy is not perfectly spherical, showing a slight elongation. There appears to be some minor disturbance in the morphology, but no obvious major merger event. The object appears relatively isolated, without nearby galaxies that appear to be interacting.
