The galaxy appears as a single, diffuse object with a smooth, nearly circular morphology. There is no apparent spiral structure or bar. The color profile suggests a dominant older stellar population, appearing more yellowish and reddish in the image. A slight elongation is observed, but it is predominantly round. The image suggests a quiescent galaxy with limited star formation activity. There are no obvious signs of a major merger, but subtle distortions possibly point to minor gravitational interactions. Overall, it resembles an elliptical galaxy, potentially undergoing passive evolution.
