The galaxy presents a clear disk morphology, viewed almost perfectly edge-on. A prominent bulge, elongated along the major axis, dominates the central region. This bulge exhibits a yellowish-orange hue, suggestive of an older stellar population. The disk itself appears relatively smooth, displaying a gradient in color. The regions closest to the bulge show similar yellowish-orange coloring, while the extreme edges of the disk trend towards a bluer tint. This color difference may indicate ongoing star formation in the outer regions of the disk. There is no evidence of strong spiral arm structure. The disk extends significantly from the bulge, resulting in an elongated overall appearance. There is some evidence of minor tidal disturbance. There is no clear indication of an active galactic nucleus.
