The galaxy appears as a centrally concentrated, nearly circular object. Its light profile suggests a relatively smooth and featureless structure. The central region exhibits a bright, well-defined core. There is an absence of prominent spiral arms or a disk-like structure within the limits of the image resolution. This suggests that it is an elliptical galaxy, or a lenticular galaxy observed face-on. No obvious tidal features or signs of recent major mergers are detected. There might be some minor disturbances to the galaxy's structure. The color profile shows a relatively uniform distribution. The red color suggests it is a relatively old, passively evolving system, with little ongoing star formation. 
