The galaxy appears to be a relatively compact and smooth system, displaying a centrally concentrated luminosity profile. Its overall shape is generally elliptical, with a moderate degree of roundness. There is no obvious disk component or spiral arm structure visible. No tidal tails or other signs of recent major merger events are observed, but there is some possibility of minor disturbances to the system. The galaxy exhibits a red color, suggesting a population dominated by older stars with relatively little ongoing star formation. 
