This galaxy presents as a spiral type. Its disk is not perfectly edge-on, exhibiting a degree of tilt that allows observation of its spiral structure. The spiral arms appear loosely wound and two-armed, emanating from a central bulge of moderate size. The color gradient suggests ongoing star formation within the arms, indicated by bluer hues. The central bulge presents a smoother, yellowish color indicative of an older stellar population. There is no visual evidence of strong bar structure across the central region of the galaxy. No major merger events are evident, though subtle irregularities within the arms might suggest minor gravitational interactions or disturbances. Overall, the galaxy appears as a relatively undisturbed, actively star-forming spiral galaxy.
