The galaxy presents as a predominantly smooth object, with a hint of elongation. Its morphology is best described as intermediate in roundness, neither perfectly spherical nor highly flattened. There is little evidence of significant ongoing mergers or major disturbances; though the image quality isn't very high, it may have undergone a minor disturbance at some point. Its color profile suggests that it is predominantly composed of older stellar populations, emitting strongly in the redder parts of the spectrum.
