The galaxy presents as a centrally concentrated system with a smooth, largely featureless morphology. It appears elliptical, displaying a moderate degree of roundness. The galaxy exhibits a color gradient, with the central region appearing more yellow-red, suggestive of an older stellar population. The outer regions show a bluer hue, although the color contrast is subtle. No distinct spiral arms or prominent dust lanes are visible. There is no indication of a significant ongoing merger event, though subtle disturbances in the outer halo cannot be ruled out with the available image resolution. Overall, the galaxy appears to be an early-type system at a moderate redshift.
