The galaxy presents as a yellowish, moderately concentrated spheroid. The dominant feature is a centrally located bulge that exhibits a relatively smooth light distribution. There is evidence of some asymmetry. A faint arm can be seen extending to the upper right of the galaxy, which could be the result of a minor disturbance or previous merger event. There is no definitive dust lane visible, and the spiral structure appears diffuse. The overall color suggests a relatively old stellar population. The galaxy appears to be a massive system with a moderate rate of star formation.
