The galaxy presents a generally smooth, elliptical morphology. The light is concentrated towards the center, forming a bright, dense core. The galaxy exhibits a relatively high degree of central concentration, with the intensity gradually decreasing outwards from the core, forming a halo. The shape appears somewhat elongated, exhibiting an axis of symmetry and deviating slightly from a perfect sphere. The colour profile suggests an older stellar population throughout the galaxy. There is very little evidence of dust lanes or spiral arm structures and no pronounced asymmetry or tidal features are apparent. There may be very minor disturbances, but overall, the galaxy appears to be in a relatively undisturbed state.
