The object presents as a relatively faint galaxy, likely a spiral, viewed nearly edge-on. The disk exhibits a distinct dust lane bisecting it, obscuring the galactic center. Faint reddish hues are visible along the edges of the disk, suggestive of older stellar populations or dust reddening. The central bulge appears poorly defined. There are indications of tidal features or disturbances, perhaps resulting from a minor merger event. Overall, the morphology is complex, implying a possible history of gravitational interactions.
