The galaxy presents a mostly smooth, elliptical morphology. Its core exhibits a concentrated, yellowish hue, indicating an older stellar population. Moving outward from the center, the light gradually diffuses, transitioning to a slightly bluer tint. There is a subtle elongation, suggesting a possible cigar shape rather than a perfectly spherical form. No prominent spiral arms or dust lanes are visible; however, there is a slight hint of structure in the outer regions implying minor disturbances. Overall, the galaxy appears relatively undisturbed.
