The galaxy presents an elliptical morphology, appearing as a diffuse, somewhat flattened spheroid. A central, bright nucleus is observed, with a gradual decrease in luminosity towards the outer regions. The galaxy exhibits a smooth texture, lacking prominent spiral arms or distinct structural features. There is a subtle color gradient, shifting from a yellowish hue in the core to slightly bluer tones in the outer disk. There is no apparent indication of ongoing major merging events, though a mild irregularity in the outer halo cannot be ruled out as a sign of minor disturbances. The galaxy's overall color profile indicates a mature stellar population, suggesting moderate levels of recent star formation activity.
