This galaxy exhibits a relatively smooth, elliptical morphology with a high degree of central concentration. The light distribution appears uniform, suggesting an older stellar population. The galaxy is distinctly round in appearance, with no visible spiral arms or bar structures. There is a slight color gradient, appearing more yellow/red towards the center, indicating the presence of older, cooler stars in the core and possibly a lower metallicity in the outer regions. There is no evidence of recent major merger activity or significant tidal disturbances, as the structure appears largely undisturbed. Given its compact appearance, it is likely a massive galaxy with a high stellar mass. The lack of blue light suggests a low star formation rate.
