The galaxy presents as a relatively smooth, round object. The central region exhibits a concentrated brightness, indicative of a significant stellar population and potentially an active galactic nucleus. The light intensity gradually decreases from the core outwards. There's a subtle color gradient, transitioning from a more yellowish or golden core to slightly bluer outer regions, suggesting older stellar populations concentrated centrally and possibly more recent star formation further out. No distinct spiral arm structure or pronounced dust lanes are apparent in this image. There is a slight asymmetry, with a minor perturbation visible on one side of the galaxy, which could be a very minor disturbance within the galaxy. Overall, based on its morphology, this galaxy appears to be an elliptical galaxy.
