The galaxy appears to be an elliptical galaxy, exhibiting a smooth, largely featureless morphology with high central concentration. Its shape is predominantly round, with only slight deviations from perfect circularity. The color distribution suggests a predominantly older stellar population, shifting towards redder wavelengths in the central region, which likely corresponds to a greater density of older stars. There's a subtle greenish hue in the outskirts, which could indicate the presence of some younger stars and/or ionized gas, though these features are not prominent. There is no evidence of spiral arms, a disk structure, or ongoing major merger activity. The galaxy appears to be relatively undisturbed.