The galaxy presents as a spiral type, observed at a moderate inclination. Two prominent spiral arms emerge from a central bulge, wrapping around the galaxy. The arms appear somewhat tightly wound. The central bulge exhibits a yellowish hue, likely indicating an older stellar population. The spiral arms show a bluer coloration, suggestive of ongoing star formation regions. A strong central bar structure appears to be present. There is no immediately obvious evidence of a major merger event, although the morphology suggests some minor gravitational disturbance may have occurred, or is occurring. The galaxy's overall structure implies a disk-dominated system.
