The galaxy appears as a somewhat elliptical, diffuse object. Its color profile suggests a relatively evolved stellar population, with a dominant yellowish hue in the central region, transitioning to a redder color further out. The galaxy exhibits a smooth appearance, lacking any prominent spiral arms or significant dust lanes. There may be some minor disturbances in the morphology, but it is unclear if these are signs of a past or ongoing merger event. Overall, the galaxy seems to be a relatively massive system, exhibiting a low rate of current star formation and a high fraction of old stars. The lack of blue light indicates that there isn't much ongoing creation of new stars.
