The galaxy presents an elliptical morphology, appearing relatively smooth and featureless in the visible light spectrum. The central bulge exhibits a yellow-orange hue, indicative of an older stellar population dominated by evolved stars. A fainter, bluer disk component surrounds the bulge. There seems to be a lack of prominent spiral arm structures, and a generally homogenous structure with a slight degree of elongation. The overall appearance suggests a galaxy undergoing a quiescent evolutionary phase, with minimal ongoing star formation. There might be some minor interactions, as there is a slight visual disturbance in the outskirts.
