The galaxy presents as a somewhat smooth, centrally concentrated structure. It appears to be relatively round. The central region exhibits a yellowish hue, suggesting an older stellar population. There is a subtle gradient of decreasing surface brightness moving outward from the core. There is some slight hint of a disk-like structure, but this is fairly ambiguous. There seems to be some slight interaction or minor disturbances occurring within the galaxy, though it is not definitively undergoing a major merger. Overall it appears as a massive galaxy undergoing low amounts of star formation.
