The galaxy presents as a relatively smooth, centrally concentrated object, likely an elliptical or lenticular type. It exhibits a generally round morphology, with a slight hint of elongation. The galaxy's light profile appears to decline smoothly from the core outwards, with no obvious spiral arms or distinct features. There may be some minor asymmetries or disturbances in the outer regions, but the overall structure is dominated by the central bulge component. The core appears quite bright, suggesting a relatively high stellar density or the presence of an active galactic nucleus. The color is generally red-yellow, indicating an older stellar population and a low rate of on-going star formation. The galaxy does not appear to be undergoing a major merger, though some minor disturbances might be present.
