The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a concentrated central bulge, a gradual fading of light as you move outward from the center, which suggests a lack of significant spiral arm structure or dust lanes. The color gradient shifts from a yellowish-white core to a redder outer region, indicating an aging stellar population with less ongoing star formation. Overall the colors are on the redder side. There is the slightest suggestion of a more extended disk-like structure beyond the central region, but this is not sharply defined. There is no evidence of any major merger or significant tidal disturbance affecting the overall structure.
