The galaxy presents a clear spiral structure, characterized by two prominent spiral arms. These arms are moderately wound, displaying a morphology that is neither tightly coiled nor loosely structured. The arm structure appears somewhat flocculent, with noticeable interruptions and variations in brightness along their length. The central bulge is of moderate size relative to the disk, contributing a significant portion to the overall luminosity of the galaxy. There is no apparent bar structure. Within the arms, there are subtle variations in color, indicating regions of active star formation, most prominently blue. The galaxy overall has a fairly smooth appearance, not displaying signs of major disturbances or ongoing mergers.
