This galaxy presents as a smooth, centrally concentrated object. Its overall shape is somewhat elongated, displaying an elliptical morphology rather than a spiral structure. The color gradient suggests a relatively old stellar population, with a dominant yellowish-orange hue in the central region. There is little evidence of distinct spiral arms or dust lanes. The smooth light distribution indicates a lack of significant ongoing star formation and a generally quiescent state. No signs of recent merger events or major disturbances are apparent in its structure.
