The galaxy presents as a largely featureless elliptical system, exhibiting a smooth light distribution with a high degree of central concentration. The morphology is roughly circular, displaying minimal deviation from a rounded shape. The galaxy exhibits a color gradient, transitioning from a yellowish-orange core to a dimmer, slightly bluer outer halo. There is no visible evidence of spiral arms, bars, or significant dust lanes. It does not appear to be undergoing any major merger activity or tidal disruption. The galaxy's light profile suggests an older stellar population, as evidenced by its redder core and lack of prominent blue star-forming regions.
