This galaxy presents as a disk galaxy, viewed nearly edge-on. There is a central bulge that appears to be elliptical and somewhat elongated along the major axis of the disk. The bulge exhibits a yellowish-orange hue, possibly indicating an older stellar population. The galactic disk is visibly thin and extends significantly beyond the central bulge, suggesting substantial angular momentum.

Dust lanes appear to be present along the plane of the disk, obscuring some of the light, particularly in the central regions. These dust lanes are indicative of ongoing star formation, possibly concentrated within the disk. The disk structure is well-defined. Faint blue regions are observed at the edges of the disk, which could suggest the presence of younger, hotter stars in the spiral arms, though they are not easily discerned in this edge-on orientation.

There is no strong evidence of a significant ongoing merger or tidal disruption, though there is a very slight asymmetry to the outer disk. The overall morphology suggests a relatively undisturbed system. The lack of a pronounced bulge relative to the disk indicates a possible lower concentration of mass in the central region.
