The galaxy presents with an overall elliptical morphology, displaying a radial profile in intensity. There is an overall smooth appearance to the galaxy, but some asymmetrical disturbances in the outer regions are observed. These appear as faint plumes extending from the main body of the galaxy. These plumes are more apparent on one side of the galaxy than the other. The central region appears brighter than the surrounding area, but there is no defined nucleus visible. The light is distributed smoothly throughout. The overall color is weighted towards the green, indicating a potentially higher proportion of younger stars or ongoing star formation activity. There may be a smaller, fainter galaxy or star formation region on one side of the galaxy which seems to be affecting the overall shape.
