The galaxy appears as a centrally concentrated object, exhibiting a smooth, elliptical morphology. The light profile suggests a relatively uniform distribution of stars, with a gradual decline in intensity moving outward from the core. There is a clear dominance of older stellar populations, indicated by the yellowish-red hue of the galaxy, which suggests a low star formation rate. No spiral arm structures or significant dust lanes are discernible. The overall appearance points towards a galaxy that has largely ceased its star formation activity and is evolving passively. There are no signs of tidal disturbances or ongoing mergers.
