This galaxy exhibits an edge-on disk morphology with a prominent central bulge. The bulge appears to be relatively smooth and rounded, showing a yellowish hue, suggestive of an older stellar population. The disk itself appears thin and elongated, and its inclination is nearly perpendicular to our line of sight. There are indications of faint, blueish star-forming regions within the disk. The overall structure suggests a system with a significant stellar mass, exhibiting an estimated moderate rate of star formation. There is no visually clear evidence of major ongoing mergers, though faint disturbances cannot be ruled out.
