The galaxy exhibits a relatively smooth, oval morphology. A bright central bulge is evident, surrounded by a fainter disk. There may be some dust lanes visible, though these are not very prominent. Based on the color, the central bulge exhibits a bluer color than the disk. There is a slight asymmetry in the outer regions, suggesting a possible minor interaction or disturbance. I don't think I would classify this as a recent merger, but it could be a more distant merger.
