The galaxy presents as a somewhat elongated, disk-like structure with a relatively smooth appearance. It is oriented at an oblique angle to our line of sight. The central region exhibits a brighter, more concentrated glow, suggesting a possible bulge. The galaxy displays a bluer hue in its central and outer regions which may be an indicator of recent star formation. There may be some minor dust lanes present across the galaxy. The overall structure hints at a possible disk galaxy, though with a degree of disturbance or interaction possibly influencing its shape. No apparent signs of a distinct spiral arm structure are observed from this view.
