The galaxy presents as a largely featureless elliptical or lenticular galaxy. Its morphology is dominated by a smooth, spheroidal structure with a high degree of central concentration. The galaxy exhibits a yellow-orange hue, suggestive of an older stellar population, possibly indicating that the star formation rate is comparatively low. There is no discernible spiral arm structure or prominent dust lanes. The light distribution is quite uniform, with no obvious signs of ongoing merger events or tidal disturbances. The object appears relatively round with a slight elongation. No evidence of active galactic nucleus activity or starburst regions is readily apparent in this image.
