The galaxy presents as a singular, relatively smooth object. Its overall shape is approximately elliptical, trending toward round. The light distribution suggests a centrally concentrated mass, with intensity decreasing gradually towards the outer edges. There is a subtle color gradient observable within the galaxy's structure, with a slightly redder hue more pronounced in the core region, transitioning to a subtly bluer periphery. No prominent spiral arms or significant dust lanes are discernible. There is no evidence of any ongoing major merger events or significant tidal disturbances in its immediate vicinity. Overall, the galaxy appears to be a mature system, consistent with an early-type morphology.
