The galaxy presents a largely smooth and elliptical morphology. It exhibits a concentrated central bulge, which appears to be the dominant feature. The galaxy's overall color profile indicates a population of older stars, suggesting a relatively low rate of current star formation. There is a slight hint of a disk structure present, though it is not well-defined. No major signs of ongoing mergers or tidal disturbances are readily apparent, implying a relatively isolated system at the current time. Its apparent roundness suggests it is viewed close to face-on.
