This galaxy presents as a flattened, elongated structure, suggesting it is likely a spiral galaxy viewed edge-on or a lenticular galaxy. The central bulge exhibits a yellowish hue, potentially indicating an older stellar population with fewer hot, young stars. The outer regions of the galaxy appear fainter and display a slightly bluer color, which could be indicative of ongoing star formation. No prominent spiral arms are discernible from this view, but there seems to be a smooth, faint disk extending from the central bulge. The overall morphology suggests a relatively evolved system with no significant signs of ongoing merger activity or major disturbances.
