The galaxy presents as an elliptical-like morphology, with a smooth, centrally concentrated light distribution. The core exhibits a bright, yellowish-orange hue, potentially indicative of an older stellar population. Fainter, bluish-green extensions are observed away from the center, suggesting the presence of some younger stars. The galaxy does not present a clear spiral arm structure. Based on the color gradient, the estimated mass is relatively high, with moderate star formation. There is no immediately obvious sign of tidal disruption or major merger events, though subtle features suggest minor gravitational disturbances may be present.
