The galaxy presents as a smooth, elongated structure, likely a late-type spiral or an elliptical galaxy viewed edge-on. The color profile is predominantly yellowish-white, with a slightly brighter, more concentrated core region exhibiting a more pronounced golden hue. This suggests an older stellar population in the central bulge and possibly ongoing star formation within. The overall morphology indicates some form of gravitational disturbance or interaction, as there are noticeable asymmetries in the galactic disc. These asymmetries suggest tidal forces have potentially stretched the galaxy. The galaxy does not exhibit any obvious signs of active galactic nuclei or intense starburst activity, as indicated by the smooth color gradient and lack of bright, point-like sources within the disk. Further investigation is required to determine its precise classification and evolutionary history.
