The galaxy presents as an edge-on spiral or lenticular galaxy. It exhibits a highly flattened disk structure, with a prominent bulge visible as a central concentration of light. The bulge appears yellowish or reddish, suggesting an older stellar population. The disk component shows a distinct blueish hue, indicating the presence of younger stars and ongoing star formation. There is faint dust lane absorption. The overall morphology is smooth, indicating a lack of significant disturbances. The presence of detected HI suggests it retains a gas reservoir, and the estimated mass falls within the range expected for a typical spiral galaxy.
