The galaxy presents a mostly smooth, elliptical morphology, with a significant bulge component dominating the central region. The galactic disk is observed edge-on, exhibiting a flattened, elongated shape. A color gradient is noticeable, with the central bulge showing a yellowish-orange hue, suggesting an older stellar population. The outer regions of the disk appear slightly bluer, potentially indicating the presence of younger, hotter stars and ongoing star formation. There are hints of faint, diffuse spiral arm structures embedded within the disk, though they are not sharply defined. The overall structure appears relatively undisturbed, with no obvious signs of major mergers or significant tidal interactions.
