The observed galaxy presents as an elliptical or lenticular galaxy. It exhibits a smooth, concentrated central bulge that gradually fades into a diffuse halo. The galaxy's color is predominantly yellow-orange, suggesting an older stellar population with relatively little ongoing star formation and a higher proportion of evolved stars. The galaxy appears to have a somewhat elongated shape, displaying an axial ratio of approximately 0.7, with the major axis oriented roughly along a northwest-southeast line. No distinct spiral arm structures or dust lanes are visible. The overall structure appears relatively undisturbed, lacking evidence of major mergers or tidal interactions.
