The galaxy appears as a relatively smooth, elliptical or lenticular system, displaying a concentrated central bulge. The light distribution is dominated by older stellar populations, evidenced by its redder color. There is no apparent spiral arm structure or significant dust lane obscuration. It is a large and massive galaxy with very low star forming activity. There is no strong evidence of recent or ongoing merger events. The overall morphology suggests a galaxy that has largely exhausted its gas supply and transitioned to a more quiescent state. The galaxy exhibits an intermediate ellipticity, appearing neither perfectly spherical nor highly elongated.
