The galaxy presents as a face-on spiral with a moderate inclination. It exhibits well-defined spiral arms extending from a slightly prominent central bulge. These arms appear tightly wound across most of the galaxy. The central bulge displays a relatively smooth and concentrated distribution of light, with a noticeable radial gradient fading into the disk. The disk structure shows evidence of active star formation, with patchy regions of blue color likely indicating populations of young, hot stars. There is an apparent lack of a strong bar structure. No significant merger events or tidal disturbances are readily visible; the morphology seems mostly undisturbed. Overall, the galaxy exhibits a classic spiral morphology with clear signs of ongoing star formation.
