The galaxy presents as an elongated, disk-shaped system viewed nearly edge-on. A central bulge appears prominent and exhibits a yellowish hue, possibly indicating an older stellar population. Moving outward from the bulge, the disk displays a gradient in color and intensity. Closer to the bulge, the light is predominantly yellow, suggesting a continuation of the older stellar population from the bulge. The disk's outer regions show some hints of a bluer color, which may indicate ongoing star formation. No spiral arm structures are clearly visible, but subtle variations in light intensity could suggest underlying features. Overall, the galaxy exhibits a smooth, relatively undisturbed morphology.
