The galaxy presents an elliptical morphology, appearing largely smooth and well-defined. A concentrated central bulge is evident, characterized by a yellowish hue, indicative of an older stellar population. There is little evidence of distinct spiral arms or significant dust lanes. The overall color gradient suggests a relatively passive galaxy with limited ongoing star formation. The galaxy appears relatively undisturbed, without major signs of interaction or merging events. The roundness suggests a high degree of intrinsic symmetry in its overall structure.
