The galaxy presents a largely smooth, elliptical morphology, showing a high degree of central concentration. The light distribution suggests an absence of prominent spiral arms or a well-defined disk structure. The color profile indicates a generally older stellar population, with a yellowish-red hue dominating the core. However, there appears to be some bluer light mixed in, indicating the presence of at least some younger stars. There is no evidence of significant ongoing merger activity or major disturbances within the galaxy's structure. Overall, the galaxy appears to be a relatively quiescent system, potentially in a later stage of its evolution. The roundness fraction is quite high, lending to the smooth appearance.
