The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The core exhibits a yellowish hue, suggesting an older stellar population. A gradual transition from the core outwards reveals a region of diffuse greenish light, possibly indicating the presence of younger stars or ionized gas. There is no evidence of spiral arms or a prominent disk structure. The overall structure appears undisturbed, with no signs of major mergers or tidal interactions. It seems relatively quiescent in terms of current star formation activity. The galaxy appears moderately round in shape.