The galaxy presents an overall elliptical morphology, although with a slight distortion suggestive of a possible disk component viewed at an angle. The central region exhibits a high concentration of light, indicating a prominent bulge or core. The light from the galactic center is a bright yellow, with the light further from the center fading into a redder hue. This color difference may suggest differing stellar populations within the galaxy; for example, younger populations towards the galaxy's center. There is some indication of irregular or distorted structure, possibly due to tidal interactions or recent merger activity. The galaxy is relatively compact in apparent size, and there is no obvious indication of significant star formation present in the overall image. 
