The galaxy presents as a centrally concentrated, elliptical-like structure. Its morphology is largely smooth, without discernible spiral arms or a prominent disk. The galaxy's core exhibits a bright, yellowish hue, potentially indicative of an older stellar population. There is a slight elongation. The galaxy appears to be largely undisturbed, showing no strong signs of major mergers or tidal interactions. Faint color variations are present in the outer regions, but not particularly intense star formation regions. The galaxy's overall structure suggests an evolved system, potentially with a relatively quiescent star formation history.
