The galaxy presents as a predominantly smooth, elliptical structure. Its central region exhibits a high surface brightness, indicative of a concentrated stellar population. Proceeding outward from the core, the luminosity gradually diminishes. The isophotes appear generally elliptical, with a moderate degree of ellipticity. A faint disk is possibly present. There is no clear evidence of ongoing major mergers or significant tidal disturbances in the immediate vicinity. A minor disturbance may be ongoing. The color profile suggests a relatively evolved stellar population with low ongoing star formation, with the central region appearing more yellow and the outer regions appearing more blue. The overall color index places it firmly within the red sequence. The size of the galaxy is moderate, neither particularly large nor exceptionally small compared to other galaxies at similar redshifts.
