The galaxy presents as a dominant, centrally concentrated object with a smooth, elliptical morphology. It exhibits a relatively homogenous luminosity distribution, lacking prominent spiral arms or distinct features. Its color is noticeably reddish, suggesting a population of older, cooler stars and a potentially lower rate of ongoing star formation activity. The galaxy's overall structure suggests it has undergone significant dynamical relaxation. There is a hint of some minor tidal disturbance and a hint of it being a merger. 
