The galaxy presents as a largely smooth, elliptical structure with a concentrated central bulge. The light profile appears relatively uniform, indicative of an older stellar population. There's a slight extension to one side, possibly a faint tidal feature or asymmetry within the galaxy's stellar distribution, but the galaxy is largely undisturbed and non-merging. The color suggests a redder hue, which is consistent with a population of older, redder stars. Its apparent size is relatively compact, with no pronounced spiral arms or disk-like features easily discernible.
