The galaxy presents as a centrally concentrated, elliptical-like structure. Its morphology appears largely smooth, lacking prominent spiral arms or significant substructure in this image. The light is dominated by an older stellar population. There may be a slight color gradient, with the central region appearing more yellowish-white, potentially indicating a higher density of older, redder stars. The outer regions fade gradually, showing a decrease in surface brightness, and a faint halo. There are no obvious signs of recent merger activity or significant star formation.
