This galaxy presents as an elliptical morphology, exhibiting a smooth, centrally concentrated light distribution. The galaxy's core appears a yellowish-orange hue, suggesting a population of older, evolved stars. The light profile appears to fade gradually from the core outwards, with no discernible spiral arms or significant dust lanes visible in this image, which supports its classification as elliptical. It is mostly rounded, but slightly elongated. There is no indication of active galactic nuclei or recent major merger events in this image; overall it appears to be a relatively quiescent system.
