The galaxy presents as a centrally concentrated, largely featureless object. It appears spheroidal in shape, exhibiting a smooth light distribution with a high degree of central concentration. The galaxy's core displays a yellowish hue, possibly indicating an older stellar population. The outer regions appear more diffuse, gradually fading into the background sky. There's no discernible evidence of spiral arms, bars, or significant dust lanes. No apparent major tidal disturbances or signs of an ongoing major merger event are observed. Subtle asymmetries or minor disturbances are not obviously evident from this imagery.
