The galaxy presents a prominent disk structure, exhibiting a well-defined spiral morphology. Two distinct spiral arms are discernible, tightly wound around the central bulge region. The arms display a blue hue, suggesting active star formation within. The central bulge appears yellowish-white, indicative of an older stellar population. No bar structure is readily apparent, nor any sign of significant tidal disturbances or ongoing major mergers. The galaxy appears relatively undisturbed. The spiral arms are somewhat difficult to resolve completely due to the relatively small size and distance of the galaxy. There also appears to be some dust lanes present. 
