The galaxy presents as a smooth, elongated structure, likely an elliptical or lenticular type. A concentrated central bulge exhibits a yellowish-orange hue, suggesting an older stellar population. The outer regions are less defined and appear bluer, potentially indicating some ongoing, albeit low, star formation. The galaxy appears relatively undisturbed, showing no obvious signs of major mergers or tidal interactions. It exhibits an intermediate axis ratio and does not present a well-defined disk.
