The galaxy presents as a somewhat diffuse, centrally concentrated object. Its morphology suggests a transition state, possibly between a spiral and an elliptical galaxy, or perhaps a galaxy that has undergone some sort of disturbance. The central region appears smoother and more consolidated, with a gradual decrease in surface brightness towards the outer regions. There are hints of faint, extended features emanating from the core, indicating a potentially active region. The light emitted is more in the blue end of the spectrum. There also seems to be a possibility of merging between the two galaxies.
