This galaxy appears to be a relatively luminous object at a considerable distance. Morphologically, it presents as a system that may be undergoing a merger or experiencing gravitational interaction with another galaxy. There are two main components that are smooth and rounded. The galaxy exhibits a yellow hue, suggesting a population of older stars. The overall shape is roughly round, although some distortions are noticeable. There are possible tidal features or minor disturbances visible, indicating past or ongoing interactions that may be slightly disrupting the galaxy's structure. A lack of distinct spiral arms or features associated with younger stellar populations is apparent.
