The galaxy appears to be an elliptical or lenticular type, exhibiting a smooth, symmetrical morphology. It is characterized by a central concentration of light, yellowish in color, indicative of an older stellar population. The galaxy's light profile decreases smoothly outwards from the core without any discernible spiral arm structures or distinct features. It is roughly circular in shape, exhibiting high degree of roundness. There is no evidence of significant dust lanes or active star formation regions within the galaxy. There does not appear to be any signs of tidal interactions or ongoing merger events. Overall, the galaxy presents a quiescent and undisturbed appearance.
