The galaxy presents as a relatively smooth, centrally concentrated object. Its color appears to be predominantly yellow-red, suggestive of an older stellar population. The overall morphology appears elliptical, with a high degree of roundness. There is no apparent spiral structure or significant disk component visible in this image. It is estimated to be a galaxy of significant mass, given its distance. Star formation activity is relatively low. There are no signs of major mergers or significant tidal disturbances, although the presence of some minor disturbance cannot be entirely ruled out.
