The galaxy presents as a spiral type, though with a notable central bulge. Two spiral arms appear prominent and well-defined. The winding of the arms appears mostly tight. The central bulge exhibits a yellow-orange hue, suggesting an older stellar population. The spiral arms are bluer in color, indicating the presence of younger stars and ongoing star formation within these regions. The galaxy appears to be a relatively isolated system, with no obvious signs of a major ongoing merger, though there appears to be a disturbance in one of the spiral arms. The galaxy does not present as edge-on. There is potentially a small bar structure. Overall, the galaxy displays characteristics consistent with a spiral galaxy possessing active star formation and with a prominent bulge.
