The galaxy presents as an elliptical morphology with a smooth, largely featureless appearance. The central region is dominated by a bright, concentrated luminosity, suggesting a high stellar density in the core. There is a noticeable color gradient, shifting from a yellowish-white core to slightly redder hues in the outer regions. No distinct spiral arm structures or prominent dust lanes are observed. The outer edges appear diffuse, lacking a sharp boundary, hinting at a gradual decrease in stellar density. Overall, the galaxy seems well-defined and symmetrical, with no obvious signs of major disturbances or ongoing merging activity, although subtle asymmetries may be present.
