The galaxy appears to be an elliptical galaxy, with a smooth, symmetrical light distribution. The galaxy exhibits a dominant bulge component and little to no evidence of spiral arms or a disk structure. It exhibits a mostly featureless morphology, with a color gradient suggesting a concentration of older stellar populations, and possible presence of dust, toward the center. The shape seems to be mostly round but not quite a perfect circle, more of an oval. The galaxy does not show any signs of recent or ongoing major mergers, and it seems to be undisturbed.