The galaxy presents as a centrally concentrated, elliptical-like structure with a smooth appearance. The color profile is primarily yellow-orange, suggesting an older stellar population. The galaxy exhibits a high degree of roundness. No distinct spiral arms or a prominent disk structure are discernible. There are no obvious signs of a major ongoing merger or significant tidal disturbances. The morphology appears largely undisturbed. There may be subtle variations in the surface brightness, but the overall structure is largely homogenous.
