The galaxy presents as a somewhat irregular, slightly elongated structure. The light is predominantly distributed in a smooth fashion, with some subtle hints of underlying features. There is a central concentration of light, with a color that indicates a relatively older stellar population. Surrounding this central region, there are diffuse, fainter extensions, giving the galaxy a somewhat disturbed appearance, possibly indicative of past interactions or mergers. The overall color suggests a population mix, with the possibility of some ongoing star formation in the outer regions, but largely dominated by an older, redder population.
