The galaxy appears as a concentrated, bright elliptical. The central bulge is a dominant feature, exhibiting a smooth, relatively uniform luminosity profile. The light is strongly concentrated towards the center. There is a general absence of distinct spiral arm structures, which, combined with the color, suggests a population of older stars and a relatively low rate of on-going star formation. The galaxy shape is generally round. There is a slight potential for some disturbance, but it is most likely a relaxed system. It is a relatively massive system given its luminosity.
