The galaxy exhibits a prominent spiral structure, with two well-defined spiral arms that appear loosely wound. The arms display a mottled texture, suggesting regions of active star formation. The central bulge is small and relatively faint. Evidence of a bar structure is present but not clearly defined. The disk appears to have a slight inclination with respect to our line of sight, obscuring some of its finer details. The galaxy shows some signs of gravitational disturbance, potentially indicative of a minor interaction with another galaxy. The overall color suggests a mix of older stellar populations in the bulge and disk and younger, bluer stars in the spiral arms.
