The galaxy appears to be a spiral galaxy, viewed at a high inclination, nearly edge-on. A central bulge is visible, appearing relatively smooth and concentrated, exhibiting a bright, whitish-yellow hue. The disk is prominent, showing a blueish tint, especially at the edges, suggesting ongoing star formation. There are a few regions of enhanced star formation visible as distinct, slightly brighter knots, mostly located in the outer disk, suggesting it is not a grand-design spiral. There is no apparent bar structure. There are no obvious signs of a major merger, though some subtle asymmetry is present in the disk, potentially indicative of a minor interaction or past merger event. Overall, the galaxy displays a morphology consistent with an intermediate spiral type.
