The galaxy presents as a centrally concentrated, luminous object with a smooth morphology. It is likely an elliptical galaxy, based on its overall light profile and lack of discernable spiral arm structures. The galaxy exhibits a yellow-white hue, indicative of an older stellar population, suggesting low current star formation rates. There is potential evidence of a minor interaction or tidal disturbance as indicated by a secondary object in the galactic halo of a reddish color. The galaxy shows a relatively high degree of central concentration, as the light is mostly focused on the center of the galaxy. The relatively small angular size indicates it is likely at a considerable distance.
