The galaxy appears as a somewhat elliptical, concentrated object. Its color profile suggests a relatively older stellar population, exhibiting a yellowish-red hue, potentially indicating lower rates of current star formation. The galaxy appears largely smooth in structure, and the shape suggests it could be an elliptical galaxy. There may be some evidence of minor tidal disturbance in the outskirts of the galaxy, but no strong indication of an ongoing merger event. The galaxy has a distinct, bright center.
