The galaxy presents a generally smooth appearance with a centrally concentrated bulge. It appears to be an intermediate disk galaxy. The bulge exhibits a bluish-white hue, suggesting a population of relatively young, hot stars and modest star formation. There are faint, subtle features that appear to be subtle arm structures extending from the central bulge. These appear only as slight color and intensity variations. There is no prominent dust lane visible. Overall, the galaxy does not present any signs of significant ongoing merger activity.
