The galaxy presents a somewhat elliptical morphology with an axial ratio of approximately 0.8. There is a central bulge that appears relatively smooth and dominant. A faint, extended disk is present. The disk exhibits faint spiral arm structures. The orientation is roughly 60 degrees. The galaxy exhibits a redder color profile, especially within the bulge, indicating an older stellar population. A possible merger event is present, there is a minor amount of disturbance noted in the main body, and a secondary object. The object is redder in color.
