The galaxy presents a largely smooth, elliptical morphology with a dominant central bulge. A faint disk component may be present, although the smooth nature of the galaxy suggests that the disk is minimal. The galaxy exhibits a high degree of circularity in its overall shape. No significant tidal features or morphological disturbances, indicative of recent major mergers, are apparent. Minor disturbances may exist but are subtle. The color gradient shows a concentration of yellow light in the center which fades into red on the outer edges of the disk. The yellow may indicate older stars and a lower rate of star formation in the central regions. Overall, it appears to be a massive galaxy, residing a significant cosmological distance.
