The galaxy presents as a relatively smooth, elliptical morphology. A bright, centrally concentrated bulge dominates the visual appearance. The light distribution appears largely uniform, with a gradual decline in luminosity from the core outwards. There are no prominent spiral arms or distinct features indicative of active star formation regions are readily apparent, though a hint of a greenish hue does point to lower levels of star formation. The galaxy appears somewhat elongated, deviating slightly from a perfectly circular shape. There is no obvious sign of interactions or mergers occurring with other galaxies.
