The galaxy presents as a prominent, edge-on disk galaxy. A significant central bulge dominates the structure, exhibiting a yellowish-orange hue, suggesting an older stellar population with reduced recent star formation. The bulge appears relatively smooth and spheroidal. Extending outwards from the bulge is a flattened disk component, displaying a range of colors, from bluish to reddish, that likely indicates varied stellar populations and ongoing star formation regions within the disk. The disk is relatively thin, and its high inclination gives it a lenticular appearance. There is a suggestion of some slight disturbance to the disk's structure but nothing major. There is no obvious indication of strong ongoing merger activity.
