The galaxy presents as an edge-on spiral, with a prominent bulge and a disk extending outward. The central bulge exhibits a yellowish hue, suggesting an older stellar population. The disk, however, displays a bluer tint, indicative of ongoing star formation. The dust lane obscuring the central bulge is irregular, possibly indicating past or current tidal interactions or minor mergers. The overall morphology suggests a relatively evolved galaxy, although with significant star formation still occurring within the disk. The overall shape appears moderately elliptical, but with some disturbances, and a slight curvature is observable in the disk, hinting at a possible warp or asymmetry.
