The galaxy presents as an edge-on spiral, with a prominent central bulge. The bulge exhibits a yellowish hue, indicative of an older stellar population. Faint, blue-tinged dust lanes are visible along the galactic plane, suggesting ongoing star formation. The disk appears relatively smooth with no obvious spiral arm structure, and is elongated with a high aspect ratio. There are no indications of tidal tails or strong morphological disturbances, suggesting a lack of recent major mergers.
