The galaxy presents as a smooth, centrally concentrated elliptical. Its light profile indicates a generally spheroidal shape, although not perfectly circular. The core region shows a concentration of older stars, exhibiting a yellowish-white hue. There is minimal evidence of prominent spiral arms or significant dust lanes within the galaxy's disk. The galaxy appears relatively undisturbed, with no obvious signs of recent major merger events or tidal distortions. There may be a faint, extended halo surrounding the main body of the galaxy, contributing to its smooth appearance. Any recent star formation is minimal, consistent with an evolved stellar population.
