The galaxy appears to be a spiral galaxy at a considerable distance, presenting a face-on orientation relative to our line of sight. A prominent, bright central bulge is visible, indicating a concentration of older stars toward the center of the galaxy. Two tightly wound spiral arms emanate from the central bulge, creating a relatively well-defined spiral structure. The arms display subtle color variations, suggesting regions of ongoing star formation. However, the overall color of the galaxy seems to be dominated by older stellar populations, with a yellow/orange hue being observed in many areas. The galaxy appears to be relatively undisturbed, with no obvious signs of a recent major merger event; it looks like a late stage spiral.
