The galaxy presents a generally smooth, elliptical morphology with no immediately discernible disk structure or spiral arms. Its light profile exhibits a high degree of central concentration, appearing nearly spherical in shape. The core region is intensely bright and yellow, suggesting a high density of older stellar populations. There's little evidence of ongoing, high levels of star formation activity from this image, as indicated by the lack of strong blue colors that accompany young, hot stars. Subtle, extended diffuse emission surrounds the bright core, fading into the background sky, marking the outer reaches of the galaxy's stellar halo. There is no visible sign of any major or minor merging events. The galaxy is generally undisturbed.
