The galaxy presents as an edge-on spiral, characterized by a flattened disk morphology. A distinct central bulge is observed, exhibiting a more concentrated and rounded structure compared to the surrounding disk. Within the disk, there appear to be hints of spiral arm structure. Dust lanes are subtly visible, particularly near the galactic plane, causing obscuration of light from regions behind them. The overall color profile suggests a mix of stellar populations. The central bulge exhibits a reddish hue, potentially indicating an older stellar population. Fainter bluer regions hint at ongoing star formation. There are no obvious signs of major mergers or significant tidal disturbances.
