The galaxy presents as a relatively smooth, somewhat rounded structure. The central region exhibits a higher concentration of light, suggesting a bulge component. Fainter light extends outward from the center, indicating a disk or halo, though no distinct spiral arms or bar structure are clearly visible. There is a subtle color gradient, with the central bulge possibly appearing slightly redder than the outer regions, which have a hint of blue. The smoothness of the overall light distribution suggests the galaxy is not currently undergoing a major merger, although minor disturbances or interactions cannot be ruled out from this image alone.
