The galaxy presents as a luminous, centrally concentrated object, likely an elliptical or lenticular galaxy based on its smooth, featureless appearance. The core exhibits a yellowish hue, possibly indicative of an older stellar population and lower star formation activity. Fainter, redder extensions appear around this, suggesting a more diffuse halo. There appears to be signs of disturbance or interaction, in the form of an asymmetrical distribution of the fainter light, especially toward the outer regions of the galaxy. The overall rounded shape is evident, though there may be some deviation from perfect circularity due to the previously mentioned disturbances. It seems to be of substantial mass and luminosity.
