The galaxy presents as a centrally concentrated, elliptical form with a smooth overall morphology. It exhibits a color gradient, transitioning from a yellowish-orange core to a bluer outer region, indicating possible differences in stellar populations and age. The inner region seems to have a higher concentration of older stars. There is a hint of a flattened structure or disk component, though it is not highly pronounced. No distinct spiral arm structures are evident. There does not appear to be a clear indication of any major ongoing merging activity, though minor disturbances cannot be entirely ruled out. The galaxy appears to be relatively isolated in its immediate environment. The overall smooth appearance suggests it is a mature system that has undergone significant evolution.
