The galaxy presents a generally smooth morphology, with a dominant, bright central bulge. The light from the bulge appears golden or yellowish. There is a subtle disk component present, extending outwards from the bulge. It appears somewhat disturbed or possibly interacting, showing hints of tidal features or minor irregularities. Overall, the shape of the galaxy leans towards being more oval than perfectly spherical. There is no strong evidence of major ongoing merger activity, but subtle distortions suggest potential past interactions.
