The galaxy presents as a smooth, centrally concentrated object with an ellipsoidal morphology. Its core exhibits a yellow-white hue, suggesting a population of older stars. Extending outwards from the core is a diffuse, bluish halo, which may indicate ongoing or recent star formation activity. The overall form of the galaxy appears relatively undisturbed, with no obvious signs of tidal tails or major mergers. There is a slight asymmetry in the outer regions, but its origin cannot be confidently determined from this image alone. The galaxy is reasonably well defined with a clear edge, with faint outer reaches. The majority of its mass seems to be located in the center of the galaxy as indicated by the high concentrations of brighter light there.
