The galaxy presents as a generally smooth, centrally concentrated object with an elliptical morphology. It exhibits a high degree of roundness, with an axis ratio approaching unity. There is no strong evidence of spiral arm structure or a well-defined disk. The central region displays a bright, yellowish core that fades into a surrounding halo. There are only minor irregularities or disturbances in the galaxy's overall structure, suggesting it is not undergoing a major merger event, but possibly shows signs of a minor disturbance. The color gradient suggests an aging stellar population with ongoing, low-level star formation activity within the galaxy. Overall, this galaxy appears to be a relatively evolved system.
