This galaxy appears to be an elliptical or lenticular type, exhibiting a relatively smooth and concentrated light profile. There are no readily discernible spiral arms or prominent dust lanes. The galaxy displays a somewhat elongated morphology, deviating slightly from a perfectly circular shape. Its color index suggests a redder, more evolved stellar population, indicative of potentially lower current star formation activity. There is a slight disturbance to the smoothness of the galaxy, suggesting it may be undergoing a minor interaction or disturbance, however there are no indications of a major merging event. Overall, this galaxy presents as a massive, quiescent system observed at an intermediate redshift.
