The galaxy appears as a relatively smooth, elliptical-like structure with a central bulge that exhibits a yellowish hue, suggesting an older stellar population. The outer regions of the galaxy display a bluish tint, potentially indicating more recent star formation. There are hints of a possible disk-like component, but the overall morphology suggests a transition between a pure elliptical and a spiral galaxy. There is no noticeable disturbance or merging features, suggesting it is in a relatively quiescent state. The shape is observed to be slightly elongated, not perfectly spherical, with an intermediate roundness.