The galaxy appears as a single, concentrated luminous entity. It presents a largely featureless morphology, exhibiting a smooth and centrally concentrated light profile. The overall shape approximates a flattened spheroid, appearing more elliptical than circular in projection. The light distribution reveals a relatively uniform color gradient, transitioning from a slightly bluer central region to a redder outer halo. No distinct spiral arms or bar structures are discernible. There is no evidence of ongoing or recent major merger activity, though minor disturbances cannot be completely ruled out based on visual inspection alone. The galaxy exhibits a modest degree of star formation.
