The galaxy presents as a moderately luminous, elongated object, likely an elliptical or lenticular type. Its color is predominantly yellow-orange, suggesting an older stellar population with lower levels of ongoing star formation. There is a smooth and featureless appearance to the galaxy. No distinct spiral arms or dust lanes are discernible in this image. The morphology of the galaxy is indicative of a system that has undergone significant merging or internal relaxation, resulting in a spheroid dominated structure. The lack of visible disturbance suggests it is not currently undergoing major interactions with other galaxies.
