The object presents as a spheroid galaxy, exhibiting a predominantly smooth morphology, and has a redshift suggesting it is relatively distant. The galaxy appears to be slightly elongated, but broadly elliptical, with a distinct central bulge that dominates the light profile. The color suggests an older stellar population, with less blue light indicative of ongoing star formation, and greater presence of redder, evolved stars. Overall, this galaxy is a massive early-type galaxy at moderate redshift with very little star formation. It could be that this galaxy is in the process of merging with a smaller satellite galaxy which is nearby the main galaxy, but there is not major distortion present.
