The galaxy presents as a primarily smooth, elliptical structure, exhibiting a concentrated central bulge that gradually fades into the surrounding halo. The core appears a bright yellowish-white, suggesting a relatively older stellar population. Moving outward, the color transitions to a slightly redder hue. There's a subtle suggestion of an extended stellar halo, though no distinct spiral arms or other features are apparent. The overall morphology suggests a galaxy that has undergone significant evolution, possibly nearing the end of its star-forming period. There are no obvious signs of recent or ongoing mergers, indicating a relatively undisturbed evolutionary history.
