The galaxy presents as a centrally concentrated, elliptical morphology, exhibiting a smooth luminosity profile without prominent spiral arms or disk features. The core region displays a high surface brightness, appearing yellowish in color, suggestive of an older stellar population and minimal ongoing star formation. The outer regions of the galaxy fade gradually into the background, indicating a diffuse halo structure. There are no visible signs of tidal disturbances or recent merger activity. Overall, the galaxy seems to be a relaxed system with a spheroidal shape, consistent with a typical elliptical galaxy at a moderate redshift.
