The galaxy appears to be a single, relatively smooth object. It exhibits a roughly elliptical morphology, displaying a modest degree of roundness rather than a highly elongated shape. There is a bright central concentration that could possibly be the core. Evident from its coloration, the galaxy displays a moderate amount of ongoing star formation. There is no strong evidence of a major merger or significant tidal disturbances; however, there is a slight chance for a minor disturbance that could possibly be a dwarf galaxy being gravitationally attracted by the larger object.
