The galaxy appears to be an elongated spiral system oriented approximately horizontally in the image. The central bulge is not particularly prominent, appearing relatively smooth and only slightly brighter than the surrounding disk. The disk shows some evidence of spiral arm structure, though it is not well-defined. There may be some slight disturbances present, but it is primarily unperturbed. Based on its dimensions and overall appearance, this galaxy is a relatively massive system. The color indices suggest a relatively older stellar population and a low rate of star formation.
