The galaxy presents a distinct spiral structure. The spiral arms exhibit a relatively tight winding pattern, appearing somewhat flocculent rather than grand design. The dominant color is bluish, suggesting the presence of younger, hotter stars in the spiral arms. The central bulge appears moderately sized with a yellowish hue, indicating an older stellar population. Overall, the galaxy appears relatively undisturbed, with no obvious signs of major merger activity, although there may be some minor disturbances or asymmetries in the outer regions of the disk. The galaxy is viewed at an angle, though not completely edge-on, allowing the spiral structure to be clearly observed.