The galaxy presents a disk-like morphology, exhibiting a clear central bulge. The disk appears relatively smooth with little in the way of defined spiral arm structure. The object's shape is leaning towards an "in-between" roundness, more elliptical than circular. Based on the color profile, the galaxy shows a population of relatively older stars. There is a faint suggestion of a possible minor disturbance, but overall, the object appears relatively undisturbed. There is a possible dust lane near the center of the galaxy. The object's light is slightly redder than blue. The galaxy is of relatively low mass and has low star formation.
