The galaxy presents as a centrally concentrated, elliptical-like object with a smooth light distribution. It displays a yellowish-white core which indicates an older stellar population. The outer regions exhibit a subtle fading, showing a transition from yellow to red, suggesting some ongoing or recent star formation in the outer disk, but at a low rate. There are no clear spiral arms visible, nor evidence of strong dust lanes or active galactic nucleus activity in this image. Overall, the galaxy's morphology suggests a system undergoing passive evolution, with potentially a mild amount of star formation in the outer regions. There's no clear sign of tidal disturbances which indicates a lack of recent major mergers.
