The galaxy presents as a relatively smooth, elliptical or lenticular structure with a concentrated central bulge. The light profile appears to decline gradually from the center outwards, lacking any distinct spiral arms or prominent disk features. Its shape is neither perfectly round nor highly elongated, appearing somewhat flattened. The color is predominantly yellowish-white, suggesting an older stellar population with a relatively low rate of on-going star formation. The galaxy shows no obvious signs of recent major merger events or strong tidal disturbances, though a minor asymmetry or subtle irregularity in the outer regions cannot be entirely ruled out. Overall, the galaxy's morphology indicates a mature system with a significant stellar mass and a quiescient state.
