The galaxy exhibits a significant redshift, suggesting substantial distance. It appears to be an edge-on spiral galaxy, characterized by a prominent, flattened disk. The central bulge appears elongated and exhibits a slight boxy shape. There is evidence of internal structure within the disk, possibly indicating spiral arm features. The overall color gradient suggests older stellar populations are concentrated within the central bulge, with younger, bluer stars sparsely distributed throughout the disk. There is very little dust obscuration apparent. The morphology suggests a quiescent state, with no major merger events or significant tidal disturbances visibly affecting the galactic structure. The galaxy is relatively large.
