The galaxy presents as a centrally concentrated object, with a smooth, relatively featureless appearance. It exhibits a general spheroidal morphology, leaning towards an elliptical classification rather than a spiral. The color profile is dominated by redder wavelengths, with a relatively diminished presence of blue light. This suggests a population of older stars. There may be little to no ongoing star formation within the galaxy, and it is not actively undergoing a major merger. There is a very small possibility of it experiencing a minor disturbance.
