This galaxy presents as an elliptical morphology, although not perfectly spherical. The central bulge appears bright and yellowish, suggesting a population of older stars. The luminosity decreases gradually outward from the core, with a smooth transition to the fainter, extended halo. There is a very slight indication of a flattened disk structure, but it is not highly pronounced. No distinct spiral arms or significant dust lanes are visible. The overall color gradient suggests that star formation is relatively quiescent within this system. There are no apparent signs of recent major merger events, though there is a chance of a minor interaction based on a small disturbance, such as a lopsided edge.
