The galaxy presents as a smooth, elongated structure with a clear central bulge. The light distribution appears concentrated towards the core, fading gradually outwards into a less defined halo. The galaxy exhibits a color gradient, with the central regions appearing more yellowish-white, potentially indicating an older stellar population. The outer regions appear more bluish, suggesting the presence of younger stars or ongoing star formation, albeit at a low rate. There are no obvious spiral arms or strong dust lanes visible, and there are no signs of any significant tidal disturbances or ongoing major mergers. The shape is generally regular, with a moderate ellipticity, suggesting that it is most likely an elliptical or lenticular galaxy seen at an angle.
