The galaxy appears to be a relatively smooth, elliptical galaxy at a moderate redshift. It exhibits a generally spheroidal shape, with a high degree of roundness. A bright, concentrated core dominates the galaxy's luminosity profile, fading outward into a diffuse halo. There is a lack of any visible spiral arm structure or prominent dust lanes. No signs of major mergers are immediately apparent. There might be a very slight hint of a minor tidal disturbance, but it is difficult to determine without further observations. The galaxy's color suggests an older stellar population and potentially low ongoing star formation.
