This galaxy appears to be a spiral galaxy observed at an angle, likely exhibiting a disk-like morphology. It displays a prominent central bulge, characterized by a yellowish hue. The bulge may indicate an older stellar population, possibly associated with a supermassive black hole. The disk appears to be relatively faint and inclined to our line of sight, presenting an edge-on view. There is some evidence of blue star formation in the galaxy disk which is a possible indicator of on-going star formation in the disk of the galaxy. There are no significant signs of major merger activity or interactions with other galaxies. The morphology is consistent with a system that is relatively undisturbed.
