The galaxy presents an overall elliptical morphology with a high degree of smoothness. It is moderately bright, exhibiting a concentrated core region that appears to dominate the galaxy's light output. The radial light profile decreases smoothly from the core outwards with no distinct features. The galaxy appears to be slightly elongated. The color indices suggest the galaxy is composed of an older stellar population, with only low levels of on-going star formation activity. The galaxy appears to be slightly disrupted and possibly merging.
