This galaxy presents an intermediate redshift, suggesting a considerable distance. Morphologically, the light distribution appears predominantly smooth, but there is also evidence of some features or a disk-like component. The galaxy exhibits a centrally concentrated bulge surrounded by a fainter, more diffuse halo. There is a hint of asymmetry in the outer regions, potentially indicative of tidal interactions or past merger events. Color gradients across the galaxy suggest variations in stellar populations, with bluer colors concentrated in the central regions and redder colors in the outskirts. This could imply ongoing star formation in the core or differences in the age and metallicity of stars in different regions of the galaxy. There also seems to be a small indication of a dust lane present in this galaxy.
