The galaxy presents a somewhat irregular morphology. It is characterized by a centrally concentrated bulge region that emits strongly in the visible spectrum. The surrounding disk appears diffuse, with low luminosity at the visible bands, indicating it may be composed of older stellar populations and/or a low star formation rate. Evident is a degree of disturbance in the disk structure, possibly indicating an ongoing or past interaction or merger event with another galaxy. Faint tidal features might be present, but are not distinctly separated.
