The galaxy exhibits an irregular morphology. Its light profile appears somewhat diffuse, showing characteristics of a possible disk component, although it lacks clear spiral arm structures. There are some subtle color gradients across the galaxy, with slightly bluer regions interspersed with redder areas, suggesting variations in stellar populations or dust distribution. A minor disturbance in the galaxy's structure is apparent, potentially indicating a past or ongoing interaction. There are no apparent signs of a major merger event.
