The galaxy presents as a centrally concentrated object, exhibiting a smooth, elliptical morphology with a high degree of roundness. The core region displays a notably brighter, yellowish hue, suggesting an older stellar population dominates the nuclear area. The color profile transitions to a bluer, albeit faint, outer envelope. There is no discernible spiral structure or distinct features like prominent dust lanes or tidal tails, implying a relatively undisturbed state. The overall impression is that of a mature galaxy with minimal ongoing star formation.
