The galaxy presents as an edge-on spiral, exhibiting a prominent central bulge. The bulge appears relatively smooth and rounded. The disk is observed to be thin and elongated. There appears to be some evidence of dust lanes along the plane of the disk, although the resolution is not high enough to discern them clearly.

The galaxy appears to have a moderate redshift, suggesting it is at a considerable distance. Star formation is likely occurring within the disk, though at a low rate. There appears to be a disturbance or possible tidal feature extending from one end of the galaxy. This could indicate minor interaction with a nearby galaxy. The galaxy shows no signs of major disturbances or a recent major merger event. The colors suggest an older stellar population. 
