The galaxy presents as a faint, elongated structure, likely an edge-on spiral or lenticular galaxy. Its light distribution suggests a prominent bulge and a relatively thin disk. The bulge appears yellowish, indicating an older stellar population, while the disk exhibits a bluer hue, implying ongoing star formation. There is no discernible evidence of spiral arms, likely due to the viewing angle, although some features are visible. There are no signs of a recent major merger event.
