The observed galaxy presents as a disk galaxy, viewed at a high inclination. A bright central bulge is visible. The disk itself appears relatively smooth, with a color gradient suggestive of varying stellar populations. The central bulge exhibits a bluer hue, potentially indicating younger stars. The disk shows some yellowing, indicative of more intermediate age stars. Faint, diffuse spiral arm structures might exist within the disk, though the image clarity limits conclusive identification. No obvious signs of major merger events or significant tidal disturbances are observed. The central bulge seems to dominate the light output.
