The galaxy exhibits a generally elliptical morphology. Its overall light distribution appears smooth and centrally concentrated, with the highest luminosity observed at the core, indicative of a possible bulge. The galaxy has a noticeable color gradient, transitioning from a yellowish-white center towards bluer hues in the outer regions. The structure appears relatively undisturbed with no apparent signs of major mergers. Faint features resembling spiral arms or a disk structure cannot be entirely ruled out given the resolution. There is no obvious indication of an active galactic nucleus or intense star formation in the core based on the data. The red shift suggests it is a moderately distant galaxy.
