The galaxy presents as an edge-on spiral, exhibiting a prominent, elongated disk structure. The central bulge appears relatively large and luminous with a yellowish hue, suggesting an older stellar population. The disk component shows subtle color variations, with some bluer regions possibly indicative of ongoing star formation. There is little evidence of significant morphological disturbances or major mergers, though a slight asymmetry in the disk could suggest minor tidal interactions. The overall shape is smooth, with a slight warp to the galaxy disc. Dust lanes are vaguely visible along the galactic plane.
