The galaxy presents as a relatively smooth, centrally concentrated object with a somewhat elliptical morphology. It exhibits a yellowish hue, suggesting an older stellar population with a lower rate of star formation. There are no distinct spiral arm structures or prominent dust lanes visible. The overall appearance suggests a galaxy that is either an elliptical galaxy or a lenticular galaxy seen at a significant distance, corresponding to an intermediate redshift. The lack of morphological disturbances implies that it is likely not undergoing a major merger event, although minor interactions or disturbances cannot be ruled out based on this single image.
