The galaxy presents as a single, somewhat amorphous object with a generally elliptical morphology. Its core exhibits a concentrated, yellowish-white luminosity, suggesting a population of older stars. The surrounding halo, fainter and less defined, displays a more diffuse, slightly bluer coloration, potentially indicating ongoing or recent star formation activity. There are hints of subtle disturbances or tidal features in the outer regions, indicating a possibility of past interactions or mergers. Overall, the galaxy appears relatively massive with moderate star formation.
