The galaxy presents a clear spiral structure, viewed at an inclined angle relative to our line of sight. Two prominent spiral arms are wound around the central bulge. The winding of these arms appears to be moderately tight. The galaxy's nucleus is bright and elliptical. The light distribution suggests a substantial bulge component. The disk of the galaxy has a smooth texture with moderate concentrations of light in the spiral arms. A faint bar appears to bisect the central bulge. There does not appear to be significant dust lane obscuration visible in this observation. No signs of major mergers or extreme tidal disturbances are detected in the image. The color distribution seems to have a relatively yellow hue.
