The galaxy presents an overall elliptical morphology. It exhibits a smooth light distribution with no apparent spiral arm structures. The major axis is significantly longer than the minor axis, indicating a substantial ellipticity. The galaxy's core is a bright, concentrated central bulge with a yellowish hue, which suggests an older stellar population. The outer regions fade gradually, showing a smoother, less defined edge. The color gradient indicates a redder periphery in comparison to the central region. There are no obvious signs of recent mergers or tidal disturbances. The overall structure suggests a relatively evolved system dominated by an older stellar population.
