The galaxy appears to be a spheroid with a smooth, fairly uniform light distribution. It has a slight elongation and displays a central concentration of light. The color profile is somewhat red, suggesting an older stellar population and potentially reduced star formation activity. Based on its morphology, this is likely a massive galaxy. There is a secondary, smaller, and fainter object close to the galaxy that appears to be interacting with it. This interaction is causing a slight disruption of the main galaxy's structure. Overall, the galaxy appears relatively undisturbed except for the interaction with its neighbor.
