The galaxy presents as a centrally concentrated object with a noticeable degree of radial symmetry, possibly an elliptical galaxy. It has a yellowish hue indicative of an older stellar population, particularly concentrated towards the core, suggesting diminished star formation. It exhibits noticeable disturbances in its structure, possibly due to an ongoing or recent merger event, seen as irregularities in its overall morphology. The disturbances suggest potential tidal features or asymmetries. There is a possible faint extended halo surrounding the main body of the galaxy. The galaxy's relatively small angular size suggests it is at a considerable cosmological distance.
