The galaxy presents as a relatively compact object. The light distribution is dominated by a smooth, centrally concentrated component, indicative of a spheroid morphology. There is a suggestion of faint, diffuse structure extending beyond the main body of the galaxy, but no distinct spiral arms or bar features are discernible. The overall color profile indicates a population of older stars, as it appears redder in comparison to younger bluer star forming regions. A hint of recent activity appears in the blue/green light in the center. The apparent circularity of the galaxy suggests it is being viewed close to face-on. The general morphology indicates a relaxed system without evidence of a recent major merger, although there is faint asymmetricality which may point to minor disturbance.
