The galaxy presents as a spiral galaxy observed at a significant inclination, nearly edge-on. A distinct central bulge is visible, displaying a yellowish hue, indicative of an older stellar population. The galactic disk appears relatively smooth, suggesting a well-mixed distribution of stars and dust. Hints of spiral arm structure are present, although somewhat diffuse, exhibiting a bluer color, potentially from recent or ongoing star formation. The galaxy appears relatively undisturbed, with no obvious signs of recent major mergers or significant tidal interactions.
