The galaxy presents a predominantly smooth morphology, indicative of an elliptical or lenticular type. The light distribution suggests a centrally concentrated spheroid with a moderate degree of roundness. There appears to be a faint indication of some structure, potentially a disk component viewed nearly edge-on, or perhaps a slight disturbance in the overall spheroidal shape, though it doesn't appear to be a major merger. Color gradients suggest an older stellar population, as indicated by the reddish hues, and a relatively low rate of star formation. The galaxy possesses a substantial mass, typical of galaxies at its redshift.
