The galaxy presents an overall elliptical morphology, elongated in one axis. The central region exhibits a significantly higher luminosity, appearing smooth and concentrated, suggesting the presence of an older stellar population. Moving outwards from the core, the luminosity gradually decreases. Fainter and bluer regions can be observed towards the edges, hinting at the presence of some star formation activity, or perhaps younger stellar populations. The disk is fairly subtle. There are no indications of any spiral arm structures. There does not appear to be any signs of tidal disruption or interaction with any nearby galaxies. Overall, this galaxy is an elliptical galaxy with some hints of recent, though limited, star formation.
