The galaxy presents a predominantly smooth morphology, with a high degree of central concentration. The light is centrally concentrated in the core of the galaxy. It exhibits a generally elliptical shape, appearing nearly round on the sky. There is minimal evidence of spiral arm structures or significant dust lanes. The light profile suggests a relatively old stellar population with a low rate of ongoing star formation. There are no signs of tidal tails or distortions indicative of recent major merger events. A very minor disturbance in shape is possible, and there is a slight color gradient within the galaxy, becoming bluer towards the outer edges of the galaxy.
