The galaxy presents as a relatively smooth and centrally concentrated object. It exhibits an approximately round morphology. A faint, reddish plume extends outward from the main body of the galaxy. This feature is likely due to an artifact. The light from the galaxy indicates moderate star formation activity. The overall color profile suggests a population of stars that is not exceedingly young, but not exclusively old either, indicating an intermediate age stellar population. No significant disturbances or signs of mergers are apparent in the galaxy's structure, except for the previously mentioned plume-like structure that may be a minor disturbance or tidal feature.
