This galaxy exhibits a relatively smooth, elliptical morphology, with an apparent circularity, suggesting a classification towards E0-E3 on the Hubble sequence. The light profile appears centrally concentrated with a gradual decrease in brightness outwards, consistent with a bulge-dominated system. Its color is generally redder and it has little discernible dust or star forming regions. There is no clear evidence of spiral arm structures or ongoing major mergers or significant tidal disturbances. It is likely a massive quiescent galaxy.
