The galaxy presents as a disk-shaped morphology with an apparent smooth central bulge. The central region exhibits a bright, concentrated luminosity, suggesting a higher stellar density. The disk component appears less defined, showing an intermediate degree of ordered structure. The galaxy appears to be a barred spiral type, with faint spiral arms. There is evidence of a minor gravitational disturbance that is present within the disk morphology. The overall color appears intermediate, suggesting a mix of stellar populations with ongoing star formation, as well as older stellar populations. The galaxy's apparent size is relatively small, indicating that it is at a moderate distance. 
