The galaxy presents as a centrally concentrated object with a moderately smooth texture and a roughly elliptical shape. Its color profile suggests a dominant older stellar population, indicative of relatively low current star formation. Faint structural features that may be indicative of a galactic disk are observed. There are no strong indications of ongoing major merger events. There is a slight disturbance nearby that may be indicative of a minor interaction. The galaxy is likely a massive system.
