This galaxy presents a flattened, disk-like morphology, viewed nearly edge-on. The central bulge appears prominent and exhibits a yellowish hue, possibly indicating an older stellar population. Fainter, bluer light emanates from the outer regions of the disk, suggesting the presence of ongoing star formation. The disk itself shows some evidence of internal structure, though finer details are obscured by the viewing angle and distance. The galaxy appears relatively isolated, showing no obvious signs of major tidal interactions or mergers with other galaxies. Overall, the galaxy appears to be a relatively massive spiral galaxy with a significant bulge component and ongoing star formation within its disk.
