The galaxy presents as a moderately bright, elliptical-shaped object. Its core exhibits a concentrated, yellowish-white luminosity, suggesting a relatively older stellar population. There is a gradual decrease in surface brightness moving outwards from the core, forming an extended halo. The halo appears smoother in texture, with a subtle gradient in color toward the redder end of the spectrum. No distinct spiral arm structures or irregular features are discernible. The overall morphology indicates a system that is relatively evolved and quiescent, with little evidence of ongoing major star formation activity. There is no visual evidence of tidal disturbances or interaction with other galaxies. The galaxy appears to be a relatively isolated system.
