This galaxy presents a generally smooth morphology, with a possible disk component. The color gradients observed suggest a concentration of younger, bluer stars near the central region with the outer disk gradually fading into older stellar populations. There is some evidence of disturbance to the disk, but the galaxy is generally not involved in any major mergers. The overall shape is neither perfectly round nor highly elongated, appearing somewhat in between. It is a spiral galaxy that is undergoing moderate star formation.
