The galaxy presents as a spiral type, with a somewhat ill-defined structure. Two prominent spiral arms are clearly visible, although some arms are fainter than others. These spiral arms appear moderately wound, with some exhibiting a tighter configuration and others looser. The central bulge appears relatively small and indistinct compared to the overall disk, and it does not dominate the galaxy's visual appearance. A weak bar feature may be present. The disk shows evidence of ongoing star formation. Overall, the galaxy appears to be relatively isolated, displaying no strong signs of recent major merger activity.