This galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a bright, concentrated central region, indicative of a galactic nucleus. The light intensity decreases gradually from the center outward, forming a diffuse halo. There is a slight elongation, though the overall shape is predominantly round. Faint, blue-tinged regions are present in the outer areas, suggesting the presence of some younger stellar populations or areas of recent star formation. There are minor disturbances visible, it is possible the galaxy has undergone a small merger with another galaxy. The galaxy exhibits a red shift, meaning that it is relatively far away from the earth. Overall, the galaxy's morphology suggests a transition between a classic elliptical galaxy and a later stage system with some disk-like characteristics.
