The galaxy presents as an elongated, spindle-shaped structure. The overall color appears to be bluish-white, potentially indicative of ongoing star formation. There is a subtle variation in color along the major axis, possibly due to variations in stellar populations or dust obscuration. A lack of clearly defined spiral arms or a prominent bulge suggests a morphology that is either a relatively late-type disk galaxy viewed edge-on or an early-type lenticular galaxy. No evidence of a recent major merger is apparent, though a minor disturbance cannot be ruled out. The size of the galaxy suggests it is a relatively small galaxy.
