The galaxy appears to be a spiral type. The central bulge is prominent and moderately sized, exhibiting a smooth, concentrated light profile. Extending from the bulge are loosely wound spiral arms, indicative of ongoing star formation. The arms are somewhat patchy, suggesting varying densities of stellar populations and gas clouds along their length. There is no obvious strong central bar, but a weak bar may be present within the inner regions of the disk. The galaxy's disk shows a relatively high degree of symmetry. There is no readily apparent evidence of major mergers or tidal disruptions in the image, though subtle disturbances cannot be ruled out. The overall color of the galaxy suggests a mix of stellar populations, with both older, redder stars concentrated in the bulge and younger, bluer stars populating the spiral arms.
