The galaxy presents as a single, relatively smooth object. Its core exhibits a bright, concentrated luminosity, transitioning into a more diffuse halo. The overall shape appears generally elliptical, showing characteristics of a spheroid galaxy with a notable lack of defined spiral arms or intricate structures. A slight deviation from perfect roundness is observed. The color profile suggests a dominance of older stellar populations, indicated by the yellowish hue, hinting at a potential low star formation rate. There is no apparent evidence of tidal disturbances or major ongoing mergers in the immediate vicinity, suggesting relative gravitational isolation and long-term stability.
