The galaxy presents as a moderately luminous, elliptical structure. Its light profile appears smooth and centrally concentrated, exhibiting a gradual decline in surface brightness from the core outwards. The overall shape is neither perfectly spherical nor significantly elongated, appearing more of an intermediate elliptical morphology. The galaxy displays a yellow-orange hue, suggesting an older stellar population with relatively low rates of ongoing star formation. There are no apparent spiral arms or disk-like features. No obvious signs of recent merger activity or major disturbances are visible, though there might be a very subtle asymmetry.
