The observed galaxy exhibits a generally smooth morphology, with a suggestion of a possible interaction or merger event. The primary body of the galaxy appears somewhat elliptical, though with some asymmetry indicative of disturbance. A fainter, more compact structure is observed close to the primary galaxy and may be interacting with it. Overall, this galaxy appears to be relatively compact and a substantial intermediate redshift. The color profile suggests an evolved stellar population, with a reddish central concentration and a somewhat bluer, more diffuse outer region. 
