The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The light profile appears to be centrally dominant, decreasing in intensity towards the outer regions of the galaxy. The galaxy's color suggests an older stellar population, with a yellowish-red hue indicating a lack of significant ongoing star formation. There are no clear signs of spiral arm structures or dust lanes, consistent with a classification as an elliptical galaxy. The overall appearance indicates a relaxed, relatively undisturbed system, without any obvious signs of recent mergers or interactions. The smooth light distribution and color suggest a passively evolving galaxy, likely dominated by older stars.
