This galaxy appears to be a spiral galaxy, observed nearly edge-on from our line of sight. The central bulge exhibits a yellowish hue, suggesting an older stellar population. A relatively faint and thin disk is visible, with hints of blueish regions that could indicate ongoing star formation. The high degree of inclination makes it difficult to discern distinct spiral arm structure. There may be some disturbances to the morphology, possibly due to a minor merger event. The galaxy does not appear particularly smooth and there is a disk present. The bulge appears to be rounded. There is a smaller object near the galaxy which could be a minor disturbance.
