The galaxy appears to be a relatively smooth, elliptical-type galaxy with a concentrated central bulge. The light distribution is fairly uniform across the galaxy, suggesting an older stellar population. There are hints of a faint, diffuse halo surrounding the main body of the galaxy, but no obvious spiral arm structure or dust lanes are discernible. The overall color of the galaxy is slightly redder. There is no indication of any ongoing major merging activity, although minor disturbances cannot be ruled out.
