The galaxy appears to be a spiral galaxy, viewed at an angle between face-on and edge-on, with a slight inclination. Two prominent spiral arms emanate from a central region, although their exact winding is difficult to determine. There is evidence of a central bulge, estimated to be of moderate size relative to the disk. The dust lanes are visible within the disk, particularly along the spiral arms, suggesting ongoing star formation. The galaxy exhibits a barred structure, with a visible bar extending through the central bulge. The spiral arms appear somewhat loosely wound, suggesting the presence of recent star formation. No signs of major mergers or significant tidal distortions are apparent. The overall color is blueish, indicative of younger stellar populations.
