The galaxy appears to be relatively smooth and elliptical in morphology. The light is concentrated towards the center. The light becomes less concentrated towards the edges. Its shape is somewhere between round and in-between. There are no clear spiral arm structures present. The color profile of the galaxy suggests the presence of older stellar populations dominating the emission. There are no significant signs of active star formation, though faint blue tinges may be present. There is a possible minor disturbance or interaction with another galaxy suggesting a merger event in progress, or which may have recently taken place.
