The galaxy appears to be a relatively smooth, elliptical-like object. Its core presents a concentrated bright region with a yellowish hue, which fades into a broader, more diffuse outer region. The isophotes appear largely regular, with minimal signs of significant tidal disturbances or ongoing mergers, though subtle asymmetries or minor disturbances cannot be ruled out at this resolution. There is faint evidence of a disk. The overall color profile suggests a population of older stars, with only a small amount of recent star formation.
