The galaxy appears to be a spiral galaxy viewed at an angle. The central bulge exhibits a concentrated luminosity, suggesting a significant population of older stars. A disk component is visible, though its exact spiral structure is not clearly defined, there appears to be some structure when viewed in bluer wavelengths. The morphology is somewhere between a smooth elliptical and a well-defined spiral, with the disk being present. There are no signs of major mergers or extreme disturbances visible. The colors suggest ongoing but moderate levels of star formation.
