The galaxy appears to be a spiral, though the viewing angle presents it nearly edge-on. A central bulge is discernable, with a slight yellowish hue, suggesting an older stellar population. Fainter disk components extend along the major axis, exhibiting a bluish tint that hints at more recent star formation activity. The disk appears elongated and relatively smooth, and without any obvious large-scale disturbances or signs of a major ongoing merger, although some minor asymmetrical features may indicate past interaction or internal processes. The galaxy displays a relatively high level of global star formation, but with a low specific star formation rate. This indicates that it is forming new stars, but is not a starburst galaxy. The estimated mass is high, indicative of a massive system.
