The galaxy presents a smooth, elliptical morphology. Its light profile exhibits a high degree of central concentration, with a bright core that gradually fades outwards. The galaxy displays a largely spheroidal shape, appearing quite round with a slightly elongated form. There is no discernible disk structure or spiral arm pattern. The overall color is a yellowish-orange hue, suggesting a stellar population dominated by older, redder stars. There is no clear evidence of recent or ongoing star formation. The galaxy appears relatively undisturbed, without any obvious signs of tidal interactions or merging activity. Faint color gradients suggest the possibility of subtle variations in stellar population or metallicity across the galaxy.
