The galaxy presents as a relatively smooth, lenticular-like structure. It exhibits an elliptical morphology, appearing mostly featureless with little discernible spiral arm structure or prominent dust lanes. The light distribution is concentrated towards the center, indicating a central bulge. The galaxy appears to be undergoing minimal current star formation and is possibly transitioning to a more quiescent state. There is no strong evidence of a major ongoing merger event, though subtle disturbances cannot be entirely ruled out.
