The galaxy presents as a somewhat diffuse object, appearing neither perfectly smooth nor highly structured. There is evidence of a disk-like component but this is somewhat disrupted. The galaxy exhibits a slightly elongated morphology, trending toward a more intermediate shape rather than being perfectly round or extremely elongated. There may be some minor gravitational interaction occurring as some disturbance to its shape is seen, however, no major merger events are obvious. Based on the color, there may be some ongoing star formation, with the bluer light being indicative of star formation, while the redder hues may be a sign of older, redder stars.
