The galaxy appears as a centrally concentrated object with a largely smooth morphology. It presents a near-spherical shape, exhibiting minimal deviation from roundness. The color distribution reveals a redder core transitioning to bluer outer regions, indicative of varying stellar populations. This suggests an aging stellar population in the center with potentially ongoing star formation in the surrounding areas. There is no strong evidence of spiral arm structure or a prominent disk. Minimal disturbances or merging activity are discernible in the image. The galaxy seems to be relatively isolated, with no immediately apparent major interactions influencing its structure.
