The object presents as a single, somewhat irregular extended source with a noticeable clumpiness. It appears to have a somewhat diffuse halo and a brighter core. The luminosity seems to be distributed unevenly, with several brighter points indicating possible areas of higher activity or star formation. There is a suggestion of tidal features or minor disturbances in the galaxy's overall structure. A possibility of this galaxy being in the process of merging or having experienced a past interaction cannot be excluded due to the irregular shape.
