The galaxy presents a distinct spiral morphology. Its arms appear relatively tightly wound, tracing a clear pattern around a central bulge. This bulge seems modest in size compared to the overall disk, and possesses a moderate luminosity. The galaxy exhibits a slight elongation, with the major axis extending approximately twice the length of the minor axis. The overall color profile suggests a moderate amount of recent star formation, as evidenced by the presence of blue hues concentrated primarily within the spiral arms. No strong bar structure is immediately apparent within the galactic center. Finally, there is no major merging or tidal disturbance immediately visable with the image.
