The galaxy appears to be a relatively compact object, with a smooth, centrally concentrated morphology. There is faint evidence of a disk or some other feature. The primary light distribution is characterized by a relatively even color gradient from the center outwards, suggesting a stable stellar population. It does show signs of minor interactions or disturbances. There seems to be very little color variation throughout the galaxy and it seems to have no distinct merger features. It could have possibly had a past merger event with a smaller galaxy, evidenced by slight irregularities in the outer edges of the galaxy, suggesting an interaction.
