The galaxy presents as a relatively smooth, centrally concentrated object. It appears nearly circular in projection. The galaxy lacks prominent spiral arms or a defined bar structure, indicating a more spheroid morphology. There is no strong evidence of recent or ongoing major merger activity, though subtle irregularities might indicate minor disturbances. The light distribution is concentrated towards the center with a gradual falloff in intensity towards the outer edges. The galaxy exhibits a subtle color gradient, appearing slightly bluer in the core and redder in the outskirts.
