The galaxy presents as a spiral type, with a relatively compact morphology. The nucleus appears bright and concentrated, suggesting a moderate bulge component. Broad, somewhat indistinct spiral arms extend from the central region, exhibiting a medium winding pattern. The color gradients across the galaxy indicate active star formation within the spiral arms. The overall structure shows no major signs of disruption, implying a generally isolated evolution. Evident is a disk component, however, the galaxy is not presented edge-on. In its grand-design spiral structure, there is no apparent bar.