The galaxy presents as an edge-on spiral, exhibiting a flattened disk structure. A prominent central bulge is visible, displaying a smooth, concentrated appearance with a yellow-orange hue. This suggests an older stellar population dominating the bulge.

Dust lanes appear to be present within the disk, obscuring and reddening the light emanating from behind them. These lanes are not sharply defined, giving the galaxy a somewhat diffuse appearance. The overall light distribution suggests a relatively high concentration of mass towards the center, tapering off towards the outer regions of the disk.

A tidal tail or plume is seen extending outward from one end of the galaxy. This feature displays a gradient in colour, shifting from yellowish closer to the galactic center and becoming more blue further out. This suggests ongoing or recent interaction with another galaxy or an internal disturbance of some kind, leading to star formation in the tail. The outer regions of the galaxy and the plume are fainter and less defined.
