The galaxy presents as an elliptical or lenticular type, exhibiting a relatively smooth and featureless morphology. The light profile suggests a centrally concentrated bulge, surrounded by a more diffuse halo. The galaxy displays a subtle color gradient, appearing redder towards the center and slightly bluer in the outer regions. There is no obvious presence of spiral arms or prominent dust lanes. The overall structure indicates a system that is likely evolved, with a relatively low ongoing star formation rate. Subtle signs of minor disturbances may be present, possibly indicating past interactions with other galaxies.