The galaxy presents a somewhat elongated morphology. It exhibits a centrally concentrated region of higher luminosity, possibly indicative of a bulge or nucleus. The luminosity decreases gradually from the central region outwards. The overall color appears to be a relatively even mix of red, green and blue channels, indicating the presence of mixed stellar populations. There appears to be a possible minor disturbance to the galaxy morphology, perhaps from past interactions. The galaxy displays an estimated effective radius of approximately 0.5 kpc. The object is relatively small, implying it is a dwarf galaxy.
