The galaxy presents a somewhat elliptical morphology, appearing as an intermediate form between a perfect sphere and an elongated shape. The central region exhibits a strong concentration of light, appearing yellowish-white, suggesting a population of older, cooler stars. Moving outwards from the center, the light intensity decreases gradually, transitioning to a bluer hue in the outer regions. This suggests the presence of younger, hotter stars in the disk. There are no obvious spiral arms or a distinct bar structure visible in this image. The galaxy appears relatively undisturbed, with no clear signs of a recent major merger event.
