This galaxy exhibits a morphology consistent with a spiral galaxy, although it is not a grand design spiral. The galaxy presents a defined, moderately sized bulge region exhibiting a yellow-white hue, suggesting an older stellar population. A faint bar-like structure is visible, appearing to traverse a significant portion of the central bulge. The disk is prominent, with regions of spiral structure visible, though rather indistinct and patchy. The spiral arms appear somewhat flocculent. The overall color of the disk is bluer than the central bulge, indicative of younger stars and ongoing star formation within the spiral arms. No signs of major mergers were seen. Some patchiness in the disk suggests some interaction or disturbances, and the disk may be at a slight angle. Some dust lanes may be present, but they are indistinct.