The galaxy presents as an edge-on disk galaxy. A prominent central bulge is visible, exhibiting a yellowish hue, possibly indicating an older stellar population. The disk appears relatively smooth. The blue color of the disk suggests the presence of younger, hotter stars and ongoing star formation within the galactic plane. The high inclination angle obscures any spiral arm structure. There is no obvious sign of a major merger event or significant tidal disturbances. The smooth disk is most likely an indication of ongoing star formation. The central bulge has a slightly rounded appearance.
