The galaxy presents as a disk-shaped structure with a prominent central bulge. The disk appears tilted relative to our line of sight, exhibiting an oblong shape. The bulge region displays a yellowish-white hue, suggesting an older stellar population. The disk is less distinctly defined, showing hints of spiral arm structures though not sharply resolved. The overall color gradient from the bulge to the outer disk implies a radial distribution of stellar ages and compositions, with younger, bluer stars potentially residing within the spiral structures, even if not obviously visible. The galaxy appears relatively undisturbed, without any major signs of ongoing merger activity or significant tidal distortions.
