The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology suggests a mostly featureless elliptical-like structure, exhibiting a high degree of roundness. There is no obvious presence of spiral arms or a distinct disk. The galaxy has a yellow-red hue, which implies an older stellar population and a subdued rate of ongoing star formation. There's a slight indication of a minor disturbance in the galaxy's overall structure, possibly suggesting a past or ongoing interaction. The overall light distribution suggests an evolved system.
