The galaxy appears to be an elliptical galaxy, exhibiting a smooth, largely featureless morphology. Its shape is generally round, although with a slight elongation. There is a concentration of light toward the center, indicative of a central bulge. The color gradient suggests a stellar population that is relatively old. There is a minimal sign of spiral arms, and it is likely not actively undergoing a major merger. There is a subtle color variation, with the central region appearing more yellow/red and the outer regions trending toward blue/green. This color difference may suggest differing stellar populations.
