This galaxy presents as a relatively small, edge-on spiral galaxy. Its disk appears sharply inclined to our line of sight, offering minimal view of spiral arm structure. The disk shows a distinct blueish hue, suggesting the presence of ongoing star formation. There is a prominent central bulge, elongated along the same axis as the disk, and appears yellowish-white suggesting an older stellar population. The dust lane is quite distinct within the galaxy. There is no apparent interaction with other galaxies or evidence of any significant merger events. Overall, the galaxy appears to be a relatively isolated, actively star-forming system, with a substantial bulge component.
