The galaxy appears as a moderately bright, gravitationally bound system with a smooth, centrally concentrated light distribution. The morphology suggests a spheroid-dominated galaxy. There is a hint of a disk-like structure, but it's not sharply defined. The object exhibits an intermediate ellipticity, appearing neither perfectly spherical nor significantly elongated. There's evidence of ongoing or recent merging activity, indicated by subtle distortions in its shape and possibly tidal features or minor disturbances. Overall, it seems relatively massive and exhibits some signs of star formation.
