The galaxy presents as a centrally concentrated, yellowish-white object. It appears largely smooth in texture, with a slight elongation along what appears to be its major axis. There is a subtle gradient in color and brightness from the core outwards, with the central region appearing brighter and more yellow. No distinct spiral arms or significant dust lanes are discernible. There is a hint of bluer, less concentrated light in the outer regions of the galaxy. The overall morphology is consistent with an elliptical or lenticular galaxy, with the smooth, centrally concentrated light profile indicative of an older stellar population. The lack of strong features suggests a relatively quiescent system, potentially with a low rate of current star formation. There may be a minor disturbance, but further investigation into the data is needed to assess the possibility of past interactions.
