The galaxy presents a predominantly smooth morphology. There is a slight ellipticity to its overall shape, appearing more "in between" circular and elongated than distinctly round. Evidence suggests it may be a galaxy towards the more massive end for observed galaxies at its redshift. While generally smooth, there appears to be a very subtle asymmetry or disturbance in its outer isophotes, though no major interaction or merger features are readily apparent. The galaxy demonstrates a noticeable color gradient, being bluer towards the central region and gradually becoming redder towards the outskirts. This could be indicative of ongoing or recent star formation concentrated in the core, with a slightly older stellar population dominating the outer regions.
