The galaxy presents as a spiral type, viewed at a slight angle relative to face-on. It exhibits a prominent disk structure with well-defined spiral arms, though these arms appear somewhat tightly wound. The central bulge is moderate in size relative to the disk and displays a yellowish hue, potentially indicative of an older stellar population. There is a hint of a bar structure. The spiral arms are blueish, possibly indicating ongoing star formation. The galaxy does not seem to display any major merger or other disturbances.
