The galaxy appears as a largely featureless, centrally concentrated object. Its light profile suggests a smooth, elliptical morphology. The galaxy's color is skewed towards the red end of the spectrum indicating the presence of an older stellar population, the attenuation of light due to dust, or its high redshift. There's no clear evidence of spiral arms or a prominent disk structure within the resolution afforded by this image. The overall shape appears somewhat elongated but substantially rounded, without significant distortions suggesting a major merger event. Faint wisps of light may be present, but the image quality makes it difficult to determine if these are tidal features or artifacts. The galaxy exhibits a high degree of central concentration, with the brightest region located at its core.
