The galaxy presents an elliptical morphology. The light is concentrated towards the core, with a relatively smooth gradient outward, suggesting a bulge-dominated system. The overall color is slightly redder at the bottom and becomes brighter and blueish going up towards the center, then slightly downwards to the upper area. This hints at differing stellar populations and/or dust distribution within the galaxy. There is a very slight tidal feature in the area above the core. The absence of clear spiral arms indicates a lack of ongoing, large-scale star formation in a disk-like structure. The galaxy appears to be undergoing some sort of interaction.
