The galaxy presents a generally smooth morphology, appearing elliptical in shape. The core exhibits a strong concentration of light, indicating a significant stellar population. The galaxy transitions from a bright, yellowish-white center to a fainter, more diffuse outer region that appears blue tinged. There is no readily apparent spiral arm structure or distinct features suggesting a major ongoing merger event. The overall impression is of a relatively undisturbed system with ongoing, but not exceptionally high, levels of star formation. Faint hints of tidal disruption appear to be visible.
