The galaxy presents a largely smooth and rounded morphology. Its color profile exhibits a gradient, transitioning from a yellowish-white core to a slightly redder halo. There are no readily discernible spiral arms or bar structures, suggesting a lack of significant ongoing star formation in a disk-like structure. The light distribution appears relatively even, with a concentration towards the center. Overall, the galaxy appears as an elliptical galaxy with a smooth light profile and an aging stellar population. No indications of a major merger event are apparent.
