The galaxy presents an elliptical morphology, appearing relatively smooth with a high degree of central concentration. The light profile suggests a spheroid-dominated system, lacking prominent spiral arm structures or obvious disk features. The color is moderately red-shifted, indicating an older stellar population and potentially lower levels of ongoing star formation. The shape is somewhat elongated, with an axial ratio suggesting it is observed at an intermediate inclination angle. There is no visually apparent major interaction or strong tidal distortion indicative of recent or ongoing merger activity. Faint disturbances may be present, though not enough to make a definitive claim.
