The galaxy presents as a flattened, elongated structure, likely an edge-on or highly inclined spiral or lenticular galaxy. The central bulge region appears reddish-orange, possibly indicating an older stellar population or significant dust obscuration. Moving outward from the bulge, there's evidence of bluer regions mixed in with the redder light, especially along the edges. These bluer regions suggest the presence of younger, hotter stars, potentially in areas of active star formation. The galaxy appears relatively smooth, with no obvious signs of major disturbances or ongoing mergers. However, there might be subtle asymmetries or irregularities that are difficult to discern due to the image resolution and inclination.
