The galaxy appears as an elliptical or lenticular type. A concentrated, bright central bulge dominates the structure, exhibiting a smooth, yellowish-orange color. This suggests an older stellar population.

Fainter, bluer regions are present in what appears to be the outer disk, and are possibly sites of ongoing star formation. There's no clearly defined spiral structure, indicating a relatively undisturbed morphology. Overall, the galaxy displays a moderate level of activity. Faint indications of a minor disturbance may be present.

