The galaxy presents a generally elliptical morphology, appearing elongated in shape. The central region exhibits a bright, concentrated core, indicative of a significant stellar density. The light distribution gradually diminishes outwards from the core, displaying a smooth transition. There is a subtle color gradient observed, with the central region appearing slightly redder than the outer regions. The overall structure suggests a relatively undisturbed system, lacking prominent spiral arms or distinct features associated with ongoing major mergers. Some slight asymmetry is apparent in the outer disk which may be a sign of minor interaction.
