The galaxy presents as a generally smooth, centrally concentrated object. It exhibits a spheroidal morphology with a high degree of roundness. The light distribution suggests a relatively uniform stellar population throughout the galaxy’s extent. There are no apparent spiral arm structures or a prominent disk. There is a slight color gradient, with a subtle reddening towards the core of the galaxy. There is no evidence of ongoing major merger activity or significant tidal disturbances. The galaxy's overall structure is consistent with that of an elliptical galaxy with a substantial mass and moderate levels of star formation.
