The galaxy appears to be a luminous elliptical, exhibiting a smooth, concentrated morphology. The primary body presents a nearly circular profile. The galaxy displays a dominant yellow-orange hue, which is possibly indicative of an older stellar population with reduced ongoing star formation. There is a subtle suggestion of a minor, off-center disturbance in the galaxy's smooth profile, with a possible faint tidal tail or remnant feature. The system exhibits a concentration of light near the center, suggesting the presence of a core. The overall impression is of a galaxy that may be in a later stage of its evolution, potentially having undergone a past interaction or merger event evidenced by the tail.
