The galaxy presents as a somewhat flattened elliptical morphology, displaying a smooth, relatively featureless appearance. The light distribution suggests a central concentration of older stellar populations, indicated by the redder hue. A surrounding, more extended component, appearing greenish, possibly indicates a faint disk or halo structure. This outer region may contain pockets of more recent star formation, contributing to the observed color. There is no discernible spiral structure or bar. The overall morphology is suggestive of a galaxy that has largely completed its major merger history and is dominated by older stars, with some ongoing, but relatively low levels of, star formation in the outer regions.
