The galaxy appears to be a disk galaxy, viewed at an oblique angle. It exhibits a bright, concentrated central bulge, likely populated by older stars, giving it a yellowish hue. A flattened disk surrounds this bulge. The disk shows evidence of spiral arm structure, traced by bluer regions which suggest younger stellar populations and ongoing star formation. The overall color gradients indicate a transition from older, redder stars in the center to younger, bluer stars in the outer regions. There is a slight asymmetry to the disk.