The galaxy appears to be a spiral galaxy, viewed at a slight angle. The disk is clearly visible, exhibiting distinct spiral arm structure. Two main arms are present, winding moderately around the galactic center. A central bar is prominent, extending through the nuclear region. The bulge component seems moderate in size, not overly dominant, but noticeable. Star formation is ongoing, as indicated by the bluer regions within the spiral arms. There is no apparent sign of a major merger event.
