The galaxy presents a flattened, disk-like morphology. The central bulge is prominent and exhibits a bright, concentrated luminosity profile. The disk appears tilted relative to the line of sight, suggesting an inclined orientation. Some asymmetry is observed in the outer regions of the disk, possibly indicating interactions or disturbances. There is a relatively high likelihood of it being a disk galaxy. Overall, the galaxy displays characteristics consistent with a moderate-sized system undergoing active star formation.
