The galaxy presents as a single, relatively smooth concentration of light. There is a discernible core, possibly indicative of an active galactic nucleus or a high concentration of stars. The light appears concentrated and has a yellow hue. The galaxy appears to be elliptical, exhibiting very little disk-like structure. There is minimal distortion of the central shape, indicating no major merger events. The color suggests an older stellar population and relatively low levels of current star formation. It is possible that some form of minor disturbance is present, given the slight irregularity of the light. The general morphology is smooth and rounded.