The galaxy presents an overall elliptical morphology, appearing relatively smooth in structure. There is a hint of a slight disk, though the dominant feature is a centralized, spheroidal bulge. The light distribution suggests a high degree of central concentration. The colors are consistent with a moderately evolved stellar population, indicating a mixture of older, redder stars and perhaps some younger, bluer stars, though the redder populations seem to dominate. Evident disturbances exist that are suggestive of an ongoing or past merger event. The galaxy appears to be interacting with another galactic body, or is in the process of consuming an existing one. 
