The galaxy presents as a relatively smooth, concentrated object. It appears to be elliptical in shape, exhibiting a slight deviation from perfect circularity. The core region displays a bright, concentrated luminosity, possibly indicative of a prominent galactic nucleus. Moving outward from the core, the luminosity gradually diminishes, displaying a smooth gradient. There is a noticeable redder hue in the central regions transitioning to slightly bluer hues in the outer regions. No distinct spiral arms or significant dust lanes are discernible in this image, suggesting a lack of significant ongoing star formation. Overall, the galaxy's morphology suggests a relatively evolved system, possibly a quiescent elliptical galaxy with a large mass.
