The galaxy presents as a relatively smooth, elliptical-like structure, with a bright, concentrated central bulge. The light distribution appears centrally peaked, and the overall color is slightly redder, suggestive of an older stellar population. Faint traces of a disk-like structure may be present, but these are poorly defined and not prominent. There are some subtle disturbances to the general shape, but nothing that looks like an ongoing major merger event. There is no strong evidence for significant spiral arm structure or prominent dust lanes visible within this image.
