The galaxy appears as a single, relatively smooth and concentrated object. There is a general lack of discernible spiral arms or distinct features. The light distribution suggests it is mostly round, exhibiting a slight elongation. The color profile is dominated by yellow light, implying an older stellar population. A slight disturbance is present, but it is not immediately clear whether the disturbance is due to an ongoing merger event or internal galactic processes. The galaxy is not particularly blue, and the estimated star formation rate indicates this object is potentially a quiescent galaxy.
