The galaxy appears as a centrally concentrated, relatively smooth object. It exhibits a generally elliptical morphology with a high degree of circularity. There is a slight elongation, but the galaxy lacks any prominent disk-like structure or spiral arms visible in the image. The light profile appears to smoothly decline from the center outward. No distinct features of disturbance or interaction are readily apparent. A slight color gradient may be present, with a subtly bluer central region transitioning to a redder halo. This could indicate some ongoing central star formation with an older stellar population in the outer regions. The overall red color suggests a substantial population of evolved stars.
