The galaxy presents as a disk-shaped structure, viewed nearly edge-on. A prominent central bulge exhibits a relatively smooth, concentrated light distribution, indicating an older stellar population. The disk component appears thinner and fainter, displaying a mixture of colors, likely indicative of varying stellar populations and dust obscuration. There is some faint evidence of blue light in the outer disk regions. The disk shows limited resolved structure with no obvious spiral arm structure. The galaxy exhibits a moderate redshift, suggesting an intermediate distance. Overall, the galaxy appears to be a relatively undisturbed disk galaxy with a significant bulge component.
