The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The light profile appears centrally peaked, suggesting a bulge-dominated system. There is a radial color gradient, transitioning from a relatively bluer outer region to a yellower inner region. The color suggests a stellar population with a range of ages, potentially indicating ongoing or recent star formation in the outer regions and a more evolved population towards the center. There's no apparent spiral structure or dust lanes visible, although given the viewing resolution, subtle features could be present but unresolved. The overall impression is of a galaxy nearing the end of its star forming period and a high likelihood that it will be classified as an early type galaxy in the future.
