The observed galaxy presents a generally elliptical morphology with a high degree of central concentration. A bright, compact nucleus dominates the luminosity profile. Surrounding the core is a diffuse, extended halo exhibiting a noticeable color gradient, transitioning from a slightly greenish hue near the nucleus to a redder, fainter outer region. There is a subtle suggestion of a disk-like structure, although not viewed edge-on, as the morphology appears somewhat flattened. No significant tidal features or obvious signs of a major merger are discernible. The overall appearance points to a relatively evolved system, potentially an elliptical or lenticular galaxy.
