The galaxy presents as an elliptical morphology, exhibiting a high degree of central concentration. The color profile suggests an older stellar population, with a reddish-yellow hue dominating the core region. The smooth light distribution further supports the classification as an elliptical galaxy. There is a noticeable absence of spiral arms or significant dust lanes within the visible structure. The galaxy appears generally undisturbed, displaying no obvious signs of ongoing or recent major merger events. Subtle extensions of light are potentially visible around the primary body, possibly representing a diffuse halo. Overall, the galaxy appears well-defined with smooth features.
