The galaxy presents as a relatively smooth, centrally concentrated object. It appears nearly circular in shape. There is a slight color gradient, transitioning from a brighter, yellowish-white core to a fainter, greenish-blue outer region. No distinct spiral arms or bar structures are discernible. The galaxy's light profile suggests a lack of significant ongoing star formation in its central regions, with a possible increase in star formation towards the periphery. There is no obvious evidence of tidal interactions or major mergers. The galaxy exhibits a centrally concentrated morphology with a smooth overall structure, indicative of a potential elliptical or lenticular galaxy type.
