The galaxy presents a generally smooth, elliptical morphology. Its core exhibits a concentrated, bright yellow hue, suggesting an older stellar population. The galaxy's outer regions display a gradual decline in luminosity, transitioning to a slightly reddish-orange tinge. This color gradient suggests a possible radial variation in stellar population or dust content. There is no discernible spiral structure, bar, or significant tidal disturbances visible in this image, lending credence to its classification as an elliptical galaxy. The overall structure appears relatively undisturbed, although the resolution is limited, preventing a detailed analysis of finer morphological features.
