The galaxy appears to be an elliptical galaxy, exhibiting a largely smooth and concentrated light distribution with minimal visible structure or spiral arms. The galaxy's core shows a high degree of concentration in the yellow part of the spectrum, suggesting a population of older stars. The shape is roughly circular. There may be some slight irregularities present, indicating minor disturbances, which can be seen at the bottom left portion of the galaxy, though these are subtle and could potentially arise from artifacts. This could be due to minor tidal interactions, or active galactic nucleus activity. The color gradient suggests a radial change in stellar population, with a possible increasing fraction of younger stars, with ongoing star formation in the outer regions. 
