This galaxy presents as a spiral type, displaying a prominent central bulge. The spiral arms are clearly defined and exhibit a relatively loose winding pattern. A hint of a bar structure may be present across the bulge, though it is not sharply defined. The galaxy's disk is viewed at a slight angle, not quite edge-on, allowing for the spiral structure to be visible. There is evidence of active star formation within the spiral arms, indicated by the blue hue. There might be some minor asymmetry or disturbance in the outer regions, though further investigation is needed to confirm this.
