The galaxy appears to be a luminous object with a relatively smooth morphology. There is a slight hint of a disk-like structure, but the overall appearance suggests an elliptical or lenticular galaxy rather than a spiral. The galaxy exhibits a yellowish hue, implying an older stellar population dominated by evolved stars. There is some evidence of disturbance, such as a possible tidal tail or bridge, potentially indicating an ongoing or past merger event. The object is relatively compact, with a moderate size. There is some evidence of ongoing star formation, but at a low rate. It shows hints of internal structure but lacks clearly defined spiral arms. It seems to be a massive object.
