The galaxy presents as an elliptical or lenticular type, exhibiting a generally smooth and featureless structure. It appears largely spheroidal, with a slight deviation towards a more elongated form. The galaxy's light is concentrated towards the center, suggesting a high degree of central mass concentration. The core region displays a yellowish hue, potentially indicative of an older stellar population. Faint, diffuse extensions are observed, although there is little evidence of spiral arms or prominent dust lanes. There seems to be minor asymmetry on one side, suggesting potential past interaction with another galaxy. Overall, the system appears relatively undisturbed.
