This galaxy exhibits a distinct disk-like morphology, presented edge-on to our line of sight. The primary structure appears to be a flattened disk, with a significant concentration of light toward the central regions, suggestive of a bulge. There's a smooth appearance to the stellar distribution across the galaxy, however there is likely some structure that is unable to be seen from the edge-on perspective. The disk shows a slight color gradient, with a subtle trend toward bluer hues along the outer edges, indicating the potential presence of younger stellar populations and ongoing or recent star formation. The galaxy appears relatively undisturbed, displaying no obvious signs of recent major merger activity. The light emitted by the galaxy indicates the presence of old and young stellar populations, but overall, the light is fairly dim, which means that it has a slow star formation rate overall. The shape of the bulge cannot be accurately distinguished, as the galaxy is presented edge-on, therefore it is difficult to tell if the galaxy is a boxy bulge galaxy or an elliptical galaxy. 
