The object presents as a galaxy, exhibiting a generally smooth morphology with a slight elongation. The dominant light profile suggests a spheroid-like structure, possibly an elliptical galaxy, though a disklike structure cannot be ruled out. The galaxy's central region displays a concentrated luminosity. A color gradient is observed, with the central region appearing more yellow, transitioning to bluer hues in the outer regions. This could indicate a difference in stellar populations, with older stars dominating the core and younger stars present in the outer regions. There is no indication of strong tidal features or major merging activity based on this image alone, though subtle disturbances may be present. Overall, the galaxy appears to be a relatively undisturbed system, with no obvious signs of active star formation regions.
