This galaxy presents as a smooth, elliptical morphology. The light profile appears centrally concentrated, with a bright, nearly circular core that diffuses outward into a more extended halo. The galaxy exhibits a redder color, suggesting an older stellar population and potentially lower levels of on-going star formation. There are no distinct spiral arms or dust lanes visible. Faint color variations are present, but the overall structure lacks significant features, indicating it is likely an elliptical galaxy viewed from a relatively perpendicular angle.