The galaxy presents as a spiral structure with a prominent central bulge. The spiral arms are well-defined, exhibiting a tightly wound morphology. The arms display some patchiness, suggesting active regions of star formation. The bulge appears relatively smooth and concentrated. The overall color index indicates a bias toward bluer wavelengths, indicative of a significant young stellar population and ongoing star formation. The galaxy does not appear perfectly symmetrical, indicating the possibility of a minor gravitational interaction or internal disturbance. The elongation suggests that it is not perfectly face-on, but slightly inclined to our line of sight.
