The galaxy presents as a single, concentrated object, exhibiting a smooth and relatively featureless morphology. Its overall shape appears close to circular, with no obvious distortions or tidal tails indicative of recent major merger activity. The light profile demonstrates a centrally concentrated brightness distribution that fades gradually towards the outer edges. The core region emits light primarily in the yellow portion of the spectrum. There is a slightly more red color profile surrounding the core, and a very subtle color shift towards blue in the outer edges. There is no visible structure beyond the basic radial falloff in brightness. The galaxy likely is a relatively massive, quiescent system. There is a possibility of minor disturbances based on the slight color changes. Further data would be needed to determine the exact nature and composition of the galaxy.
