The galaxy appears to be a spiral, observed edge-on from our vantage point. A central bulge, noticeably brighter and exhibiting a yellowish hue, dominates the galaxy's core. Faint, extended dust lanes are visible, bisecting the galaxy's disc and attenuating the light from regions behind them. The disc itself appears relatively thin and elongated, showing subtle variations in brightness, suggesting the presence of spiral arm structure. A possible companion galaxy or background object can be observed slightly above the edge-on galaxy. The main galaxy's colour profile indicates that it is likely a relatively massive system. The edge-on orientation makes it difficult to determine the presence of active star formation regions.
