The galaxy presents a disturbed morphology, likely indicative of an ongoing or recent merger event. The light distribution is irregular. There are two main concentrations of light, possibly representing the cores of the merging galaxies. The central region appears yellowish, surrounded by a bluer, more diffuse halo. Faint tidal tails or extended stellar streams may be present, further supporting the merger scenario. Spiral arm structures are not well-defined; they may have been disrupted by the interaction. The galaxy is not seen edge on and has a slightly elliptical appearance, although the overall shape is distorted. It may or may not have a central bar, but the galaxy is distorted enough that it can not be readily observed.
