The galaxy presents as a centrally concentrated system with a smooth light profile, indicative of an elliptical morphology. The core exhibits a yellowish hue, potentially suggesting an older stellar population. There is an absence of distinct spiral arms or significant dust lanes, supporting the classification as an elliptical galaxy. The galaxy's overall shape is somewhat elongated. The estimated diameter is approximately 4 kpc. The red shift indicates it is relatively distant. Based on the morphology, there does not appear to be a recent merger. 
