The galaxy presents as a centrally concentrated object with a relatively smooth light distribution. Its color profile suggests a redder core transitioning to slightly bluer outer regions. The morphology appears largely spheroidal with minimal discernible substructure, such as spiral arms or a prominent bar. There is some indication of subtle asymmetries or minor disturbances in the outer envelope, potentially suggestive of past or ongoing interactions. The overall appearance is consistent with an elliptical or lenticular galaxy at an intermediate redshift. The size of the galaxy is consistent with relatively large and massive galaxies at this distance. Star formation rate is relatively low.
