The galaxy presents as a flattened spheroid, exhibiting a smooth overall morphology with a slight elongation. The color profile suggests an older stellar population, with the central bulge displaying a distinct reddish-orange hue. A faint greenish-yellow halo surrounds the core, potentially indicating the presence of younger stars or ongoing star formation within the outer regions. The galaxy appears relatively undisturbed, with no obvious signs of major mergers or significant tidal interactions. Its shape suggests a classification somewhere between an elliptical and a lenticular galaxy, with a high degree of central concentration. There are no visually apparent spiral arm structures.
