This galaxy appears to be a spiral galaxy, observed nearly edge-on from our vantage point. The central bulge is prominent, exhibiting a yellowish-white hue, suggesting an older stellar population within the core. The disk component is visible extending away from the bulge, displaying bluer tints toward the outer regions. This indicates the presence of younger, hotter stars, possibly associated with ongoing star formation. The galaxy's morphology appears relatively undisturbed, with no major signs of tidal interactions or recent mergers. There may be some evidence of dust lanes obscuring parts of the disk, although the resolution is insufficient to confirm this definitively. The galaxy appears to be actively forming stars, though at a moderate rate. The galaxy exhibits a substantial stellar mass.
