The galaxy appears to be an elliptical, with a relatively smooth light distribution, with a roughly round morphology, and a lack of prominent features like spiral arms or a bar structure. The galaxy exhibits a strong central concentration of light that gradually diminishes toward the outer edges. There is a subtle colour gradient, transitioning from a yellower hue near the core to a slightly bluer tint in the outskirts, possibly indicating differences in stellar populations. No obvious signs of recent major merger activity or significant tidal disturbances are observed. 
