The galaxy presents a relatively smooth morphology, indicating it is likely an elliptical or lenticular type. The light is generally distributed in a rounded shape. There is no prominent disk structure or spiral arms visible in the image. No signs of ongoing major mergers or significant tidal disturbances are apparent; however, there is a possibility of minor disturbances. The galaxy has a moderate amount of recent star formation. This galaxy has a median stellar mass of approximately 10^10.5 solar masses.
