The galaxy presents as a relatively smooth, centrally concentrated object. Its light profile suggests a dominant spheroid component. The isophotes appear mostly round. A faint disk cannot be ruled out. There is indication of possible minor disturbance in the morphological structure. The galaxy displays a moderate redshift, suggesting that it is relatively distant. Based on its color profile, the galaxy appears to have a population of relatively old stars. Overall, the galaxy appears to be a fairly massive system with a modest ongoing rate of star formation.
