The galaxy presents as a relatively smooth, elliptical form. It exhibits a concentrated central bulge that appears distinctly yellow-orange in color, suggesting an older stellar population. Fainter, diffuse light extends outwards from the core, with a subtle transition to a more reddish hue in the outer regions. No obvious spiral arm structures are visible. There are no signs of significant disturbances such as tidal tails or close companion galaxies. The overall appearance is consistent with a galaxy that is not undergoing active star formation and is dominated by evolved stars. The galaxy appears mostly round with a hint of elongation. The color gradient indicates potential metallicity variations, with higher metallicities perhaps concentrated in the central regions.
