The galaxy presents as a relatively smooth, centrally concentrated object, displaying a dominant spheroidal morphology. The core is bright, with an apparent gradual decrease in luminosity towards the outer regions. The color gradient suggests older stellar populations dominate throughout the galaxy. There is a possibility of minor tidal interactions or internal disturbances evidenced by a faint arm or plume-like structure extending from the main galactic body. The structure may be consistent with a minor merger or ongoing accretion event, as it is not clearly smooth.
