The galaxy appears to be a spiral galaxy, viewed nearly edge-on. A prominent central bulge exhibits a yellowish hue, suggesting a high concentration of older stellar populations. A faint, flattened disk extends outward from the bulge. The disk exhibits some mottled texture, possibly indicating dust lanes or the presence of spiral arms, although the edge-on perspective makes it difficult to discern definitive spiral structure. Faint blue tinges are visible along the edges of the disk, which may indicate regions of recent star formation within the galaxy. There is no obvious indication of any major merger activity or significant morphological disturbances.
