The galaxy presents as a somewhat elongated, disk-like structure, suggestive of an edge-on or highly inclined spiral or lenticular galaxy. The central bulge appears prominent and exhibits a yellowish hue, possibly indicating an older stellar population. The disk component is visible extending outwards from the bulge, and it has a bluer color. There's no clear evidence of strong spiral arm structure; the disk appears relatively smooth. There is a slight indication of disturbances in the galaxy, however, the morphology is primarily undisturbed. The system exhibits an overall mass, and a low rate of star formation activity. 
