The galaxy presents as a single, centrally concentrated object. The light distribution is relatively smooth, with the majority of the luminosity concentrated in a central bulge. The galaxy appears largely elliptical in shape, with the major and minor axes appearing similar in length. There may be some evidence of a very faint, diffuse disk component extending slightly beyond the main bulge, but this is not well-defined. The object appears to be largely undisturbed, with no obvious signs of major mergers or tidal features. There is a very slight elongation visible in its shape; it is close to being round.
