The galaxy presents as a relatively compact, disk-like structure seen at an oblique angle. A central bulge region dominates the morphology, appearing smooth and concentrated. The spiral arms are present but not well defined. The galaxy exhibits a bluer hue toward the outer edges, suggesting the presence of younger stellar populations and ongoing star formation in these regions, though at a low rate. There is some dust obscuration visible within the disk. There does not seem to be any significant merger activity or morphological disturbance.
