The observed galaxy presents a disk-like structure, oriented at a shallow angle relative to our line of sight. It is likely a spiral galaxy. There appears to be a central bulge, brighter and yellower than the surrounding disk. The galaxy has a high mass and likely a medium star formation rate. There is some hint of spiral arm structure, exhibiting some irregularities, possibly indicating gravitational interaction, but it is more likely a relatively undisturbed galaxy. The disk appears to be composed of stars and gas. The galaxy's color gradient suggests differential stellar populations, with bluer regions potentially indicating younger stars and ongoing star formation. Overall, this appears to be a large disk galaxy.
