The galaxy presents a mostly smooth, elliptical morphology. There is a bright central bulge with a relatively high concentration of light. Fainter, diffuse light extends outwards. There is a hint of a disk, although the light is diffuse and it is only barely discernable from the image. There also appears to be a slight perturbation to the galaxy shape. Overall the galaxy presents with a low level of recent or ongoing star formation. It appears that the system may be undergoing a minor disturbance or a weak merger event.
