The galaxy appears to be a relatively smooth, elliptical galaxy, displaying a concentrated central bulge. It appears to be generally round, with a slight elongation. No distinct spiral arm structure or prominent dust lanes are discernible. The color gradient suggests a population of older stars, leading to a redder appearance, with some evidence of recent star formation. There are no signs of tidal tails or morphological disturbances, thus, no major mergers. The galaxy is not exceedingly bright. The galaxy appears to be of intermediate mass and size.
