This galaxy exhibits a clear disk-like morphology. A central, bright bulge is visible, appearing approximately spherical and concentrated. The surrounding disk appears relatively thin and is oriented edge-on from our line of sight, suggesting the presence of dust. Evidence for spiral arm structure appears to be minimal. Color gradients across the galaxy indicate variations in stellar populations. The bulge appears bluer, possibly indicating younger stars, while the outer regions of the galaxy are redder, suggesting older stellar populations or significant dust obscuration. The galaxy shows only minor disturbances, with no obvious signs of tidal tails, bridges, or strong asymmetries.
