The galaxy appears to be a spiral galaxy seen at an oblique angle, possibly nearing edge-on. A central bulge is visible as a bright, concentrated region of yellowish light, suggesting an older stellar population. Extending outward from the bulge are faint, diffuse arms. A slight asymmetry can be seen within the disk, possibly indicating the presence of some minor gravitational disturbance. The disk itself exhibits a gradient in color, appearing bluer further from the core, indicating the presence of younger, hotter stars and ongoing star formation in the outer regions. The galaxy appears relatively smooth, with no obvious signs of recent major mergers or significant tidal features.
