This galaxy appears to be a spiral galaxy viewed at a considerable angle, approaching edge-on. A central bulge is visible with a yellowish-white hue, suggesting an older stellar population. The surrounding disk exhibits a bluish tint, indicative of ongoing star formation. There is some evidence of a slight disturbance within the disk, with some irregular shapes in the disk. The galaxy does not exhibit any major signs of a recent merger but there may be a minor disturbance. It is moderately bright, likely a massive galaxy, and possesses a low-to-moderate rate of star formation.
