The galaxy presents as a lenticular or early-type spiral, viewed at a significant inclination. The central bulge exhibits a concentrated, yellowish hue, suggesting an older stellar population. Surrounding the bulge, a faint, elongated disk is discernible, with subtle hints of spiral structure. The disk displays a bluer color, especially at its outer edges, potentially indicating regions of ongoing star formation. The galaxy appears relatively smooth in texture, with no obvious signs of major mergers or significant tidal disturbances, though some subtle asymmetries cannot be ruled out. The overall morphology is somewhere between elliptical and spiral, and it is relatively undisturbed.
