The galaxy presents as an elliptical or spheroidal structure, exhibiting a smooth, concentrated light profile. The core region displays a yellow-orange hue, suggesting an older stellar population with a lower rate of ongoing star formation. There is a lack of discernible spiral arm structures or distinct dust lanes, further supporting a classification as an elliptical galaxy. The overall morphology is characterized by a high degree of roundness and a lack of significant tidal disturbances or merging features. The galaxy appears relatively isolated and undisturbed. The estimated size is approximately 8 Kpc.
