The galaxy presents a smooth, elliptical morphology. The light profile suggests a significant bulge component, with the luminosity concentrated towards the center. There is little evidence of spiral arm structure or significant dust lanes. The overall color appears slightly redder, potentially indicating an older stellar population with a low star formation rate. The galaxy exhibits a moderate ellipticity, appearing elongated rather than perfectly spherical. There is no obvious evidence of ongoing merger activity or tidal disturbances, suggesting a relatively quiescent state.
