The galaxy presents as an elliptical morphology, appearing largely smooth and rounded in shape with a dominant central bulge. The light profile is centrally concentrated, exhibiting a gradual decrease in intensity towards the outer regions of the galaxy. A subtle extension or minor disturbance may be present on one side, though the main body of the galaxy appears undisturbed. The galaxy's color suggests an older stellar population; the dominant yellowish-orange hue indicative of evolved stars. Star formation rates appear to be suppressed.