The object presents as a spiral galaxy at a redshift of approximately 0.14. The galaxy is viewed at a slight angle, between face on and edge on, with an inclination that permits some observation of spiral arm structure. These arms are prominent and tightly wound, with a dominant two-arm structure. A weak bar is visible, extending from the central bulge. The bulge is moderately sized, occupying a significant portion of the galactic disk. The arms display a patchy texture, indicative of regions of active star formation. There is no obvious strong evidence of a major merger event although there may be minor disturbances within the galaxy. The disk color exhibits a gradient with a bluer hue in the outer regions and a redder hue closer to the center.
