The galaxy presents as a roughly elliptical structure. The central region displays a brighter core, surrounded by a more diffuse halo. A dust lane is observed across the midsection. A small tail-like formation extends off one side. Overall the galaxy appears to be undergoing some form of interaction or disturbance, with the possibility of minor disruptions to its overall morphology. The galaxy has a bluish color, which may indicate the presence of younger stellar populations.
