The galaxy appears to be an elliptical galaxy due to its smooth and largely featureless morphology. It exhibits a spheroidal shape with a concentrated, bright central bulge that fades into a more diffuse halo. The core region displays a yellowish color, possibly indicating an older stellar population. A greenish tint is present in the outskirts, potentially resulting from a lower abundance of redder stars or the presence of ionized gas. There appears to be a lack of defined spiral arms or dust lanes, confirming its classification as an elliptical galaxy, rather than a spiral galaxy. The overall structure suggests a relaxed and well-mixed stellar population, indicative of minimal ongoing star formation and little evidence of interaction or merging activity.
