The galaxy presents as a centrally concentrated, relatively smooth object with a largely spheroidal morphology. There is a noticeable color gradient, with a brighter, slightly bluer core fading into a redder halo. While the galaxy appears generally smooth, there are hints of subtle substructure or diffuse features in the outer regions. The object exhibits a roughly circular profile, with only a slight deviation from perfect roundness. There is no obvious indication of tidal interactions or major mergers, though some subtle perturbations could potentially be present upon further inspection. Overall, it seems to be an early-type galaxy with a predominantly old stellar population.
