The galaxy appears to be a relatively smooth, elliptical-type system. Its light distribution exhibits a centrally concentrated profile, fading outwards in a gradual manner. There's a hint of a more concentrated core region surrounded by a broader halo. The galaxy is generally round in appearance. The color is predominantly a yellowish-orange hue, which suggests a population of older stars dominates the stellar content, with relatively little ongoing star formation. There is no discernible spiral arm structure or strong dust lane features visible. The overall structure suggests a relaxed morphology, without evidence of significant recent mergers or interactions. The galaxy appears to be relatively isolated, with no obvious nearby companions in the immediate vicinity that would suggest tidal disturbances.