The galaxy presents a generally smooth morphology, with a high degree of central concentration. Its shape appears to be somewhere in between round and elliptical. There are hints of disturbances in the galaxy, with some slight asymmetry. The galaxy has a bright central region which suggests a higher stellar density and possibly ongoing or recent star formation. Colors indicate a mixed stellar population. There appears to be a presence of bluer light in the extended regions of the galaxy, possibly indicating younger stars. Fainter redder light is visible in the nucleus.
