The galaxy presents as a flattened, elliptical shape with a distinct central bulge. The color gradient suggests a concentration of older stars toward the core, indicated by the yellowish-white hue. The outer regions exhibit a bluer tint, possibly indicating ongoing or recent star formation. There are no clearly defined spiral arms visible. The galaxy appears relatively smooth, with some minor indications of disturbance along its edges, though no major mergers are obvious. It is neither perfectly round nor particularly elongated, appearing between these shapes. Overall, the galaxy appears to be relatively massive.
