The galaxy presents as a moderately bright, elliptical form with a high degree of central concentration. Its apparent shape suggests a roughly circular projection with a minor axis ratio indicating some flattening. The galaxy exhibits a smooth light distribution, lacking any obvious spiral arms or distinct features. Color gradients are subtle, with a generally redder core transitioning to slightly bluer outer regions. The overall color indices suggest a relatively evolved stellar population. The galaxy's size, while seemingly compact, is consistent with that of a dwarf or intermediate-mass galaxy at its estimated distance. There is no evidence of tidal disturbances or recent merger activity in the visible light.
