The galaxy presents as an edge-on or nearly edge-on spiral. The central bulge is prominent, exhibiting a yellowish-orange hue, which suggests an older stellar population. The disk component appears relatively thin and elongated. There's faint evidence of some disturbances in the disk, but no major merging events appear to be happening with this galaxy. The central bulge is rounded in shape. There is a smooth quality to the galaxy, without exhibiting distinct features like spiral arms or prominent dust lanes. 
