The galaxy appears as a central, diffuse object. It is somewhat smooth in appearance, with a slight elongation. The color suggests it is a relatively mature galaxy, with a significant population of older stars. There is a faint, extended halo of light surrounding the main body. There is no evidence of a prominent disk structure. There also isn't a bright central bulge. There is no clear evidence of a major ongoing merger event, although some minor disturbance or interaction may be present.
