The galaxy presents as an elliptical system exhibiting a smooth overall morphology. It is characterized by a centrally concentrated luminosity profile, with a gradual decrease in surface brightness towards the outer regions. The galaxy appears somewhat flattened. The central region shows a yellowish hue, potentially indicating an older stellar population dominating the core. There is evidence of bluer regions, possibly hinting at some star formation activity. Based on the overall appearance, the galaxy appears to be of considerable mass. There are some slight distortions possibly suggesting gravitational interactions. The galaxy has a red shift of approximately 0.13.
