The galaxy presents as a generally smooth, elliptical-like object with a concentrated central bulge. There is a slight elongation in its overall shape, deviating minimally from a perfect sphere. The core region exhibits a brighter, more intense luminosity, fading gradually into the surrounding halo. Subtle color variations are detectable, with a possible hint of bluer tones around the center. Fainter, diffuse extensions appear to surround the main body of the galaxy, suggesting a halo of older stellar populations. No distinct spiral arms or prominent dust lanes are visible.
