The galaxy presents as a relatively smooth, centrally concentrated elliptical type system. It exhibits a bright core region, suggesting a concentration of older stellar populations. The galaxy is elongated, with a roughly cigar-shaped morphology, although the system is mostly smooth. The overall color appears to be composed of older stars, emitting in longer wavelengths, possibly from low to moderate star formation occurring within the galaxy. No major disturbances are apparent, indicating a gravitationally settled state.
