The galaxy presents as a somewhat irregular spheroid. The light distribution is centrally concentrated, with a smooth profile suggesting an older stellar population. The galaxy exhibits a slight ellipticity but is mostly round. There is a hint of minor disturbance in the overall form, potentially indicating a past interaction or merger event. Star formation is generally low. It's overall color suggests it contains mostly older, redder stars. There is a possibility of a faint tidal tail or streamer extending from the main body of the galaxy in one direction. The estimated size of the galaxy is several kiloparsecs.
