The galaxy appears to be an elliptical galaxy with a relatively smooth morphology. It exhibits a concentrated central bulge that fades gradually towards the outer edges. The color appears to be a yellowish-orange hue, indicative of an older stellar population. There is little evidence of spiral arms or significant dust lanes, reinforcing its classification as an elliptical galaxy. The galaxy shows no obvious signs of interaction with other galaxies, such as tidal tails or distorted shapes. The overall structure suggests a system that has largely completed its merging history.
