The galaxy presents as a centrally concentrated object with a diffuse, extended halo. The core exhibits a bright, relatively smooth appearance. The overall shape approximates an elliptical form, trending toward round, though not perfectly spherical. There is a subtle deviation from perfect smoothness, with hints of faint, internal structure potentially indicating minor disturbances. No obvious spiral arms or bar features are discernible. Overall, the galaxy does not display clear evidence of ongoing major merger activity, though a slight asymmetry may point to past or subtle gravitational interactions.
